The galaxy presents a generally elliptical morphology, exhibiting a smooth, diffuse light profile with a prominent central bulge. The core appears concentrated and is characterized by a yellow-white hue, possibly indicating an older stellar population and a relative lack of ongoing star formation. The overall color gradient shifts from a warmer yellow center to slightly cooler, bluer tones in the outer regions. A faint, diffuse halo is visible, extending beyond the main body of the galaxy and fading into the background sky. There is a potential minor interaction or merging event with a smaller, fainter object near the lower part of the galaxy, subtly disrupting the smooth light distribution. The bulk of this object presents a blue tint, potentially showing regions of star formation.
