The galaxy presents as a spiral type, viewed at a significant inclination. Its central bulge appears moderately sized, exhibiting a yellowish-white hue, suggestive of an older stellar population. Diffuse spiral arms emanate from the central region, displaying a somewhat patchy and flocculent structure. The arms exhibit a mixed color profile, with some areas showing bluer tinges indicative of more recent star formation, while other regions appear more yellowed, implying a higher proportion of evolved stars. The overall morphology suggests a relatively well-defined disk structure, although the inclination obscures detailed arm features. There is no apparent evidence of a prominent bar structure. The outer regions of the disk show signs of disturbance, possibly from minor interactions. The galaxy doesn't appear to be undergoing a major merger event, though subtle asymmetries in the outer disk could indicate past interactions or minor disturbances. Based on observed color gradients, the galaxy likely exhibits on-going star formation, with a noticeable concentration in the spiral arms.
