The galaxy presents an overall elliptical morphology, though with some suggestions of a disk structure viewed at a significant angle. The color distribution appears to have a central concentration of yellow-red hues which suggests an older stellar population. The periphery is more diffuse and slightly bluer, possibly indicating some ongoing, though subdued, star formation activity. There is no clear evidence of strong spiral arm structures or a pronounced bar. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or recent mergers, despite the presence of nearby bright objects that could appear as possible merger candidates, though they are most likely foreground stars. The galaxy's light profile is smooth with no significant knots or HII regions visible in this image.
