This galaxy presents a morphology consistent with a spiral or lenticular type, although the resolution limits precise classification. The central bulge appears prominent and exhibits a yellowish hue, suggestive of an older stellar population. A disk is faintly visible extending outwards from the bulge with a bluish tint. This may indicate regions of more recent star formation. Some degree of disturbance is present in the outer regions of the galaxy's disk. There is no clear presence of a bar structure. Overall, it's a reasonably large galaxy with a notable bulge and relatively mild star formation.
