The galaxy presents an apparent morphology exhibiting characteristics of both a smooth spheroidal component and a structured disk. The spheroidal component, likely a bulge, displays a relatively uniform brightness distribution with a yellowish hue. The disk component appears somewhat disrupted and shows possible signs of tidal features.

There is evidence to suggest a potential ongoing or recent merger event. The overall structure is disturbed, and the light distribution does not conform to a simple spiral or elliptical model. There are indications of star formation, with a bluer component visible in the disk suggesting the presence of younger stellar populations. However, star formation may be relatively quiescent based on the overall color and lack of prominent HII regions.
