The galaxy presents a generally smooth and concentrated morphology. The central bulge region exhibits a yellow-orange hue, suggestive of an older stellar population. A disk component is discernible, though less prominent, with a fainter, bluer color distribution extending outward from the bulge. There is a subtle indication of some structural disturbance, possibly an early stage merging event. The apparent ellipticity of the galaxy suggests it is an oblate spheroid. The galaxy appears to be relatively isolated, although there is some evidence of tidal interactions or minor disturbances.
