The galaxy presents as a moderately inclined, disk-shaped structure. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue, suggesting a population of older stars. Moving outwards from the bulge, a relatively smooth disk is observed, with a bluish tint indicative of ongoing star formation. The disk lacks distinct spiral arm structures and appears somewhat patchy in its color distribution. The galaxy has a slight elongation, with the major axis extending approximately twice the length of its minor axis. The overall morphology suggests a galaxy undergoing a quiescent period of star formation, without major disturbances or interactions.
