The galaxy presents a disk-like morphology, viewed at a slight angle, but not quite edge-on. Faint spiral arm structures are visible, indicating a likely spiral galaxy classification. The central bulge appears moderately sized, exhibiting a smooth, concentrated brightness profile. The galaxy displays a general blue hue, suggesting the presence of younger stellar populations and ongoing star formation. There is some indication of minor disturbances in the outer disk, possibly due to a past or ongoing interaction.
