The galaxy presents as an elliptical morphology, elongated along its major axis. Its central bulge exhibits a brighter, more concentrated luminosity profile, with a yellowish-white hue indicative of an older stellar population. Fainter, bluish extensions are observed away from the bulge, possibly suggesting some level of star formation activity in the outer regions. The overall structure appears smooth, with no readily discernible spiral arms or other distinct features. The galaxy appears to be isolated, with no obvious signs of tidal distortion or interaction with neighboring galaxies.
