The galaxy presents as a single, relatively smooth object with an elliptical morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge component. The dominant color is a yellowish-orange hue, indicative of an older stellar population and potentially a lower rate of ongoing star formation. There is little evidence of spiral arms, dust lanes, or significant irregularities in the galaxy's structure. No signs of tidal tails or merging events can be seen. The overall appearance suggests a system that is relatively evolved and quiescent.
