The galaxy presents a generally smooth, elliptical morphology. Its overall shape is approximately spheroidal, showing a slight elongation, but lacking any obvious spiral arm structure or prominent disk features. A bright, concentrated core region dominates the galaxy's luminosity profile, gradually fading into a more diffuse halo. The galaxy exhibits a color gradient, transitioning from a yellow/orange hue in the core to a redder, more subdued coloration in its outer regions. There is no clear evidence of ongoing major merger events, though a slight irregularity in the outer halo could suggest minor tidal interactions or accretion events in the galaxy's past. No prominent dust lanes or distinct star-forming regions are apparent within the observed light.
