The galaxy presents an elliptical morphology, elongated along a major axis. Its light profile suggests a relatively smooth distribution, transitioning gradually from a concentrated central region to a fainter, diffuse outer halo. The color gradient shows a concentration of yellowish hues towards the center, which may indicate an older stellar population dominating the core. The outer regions exhibit bluer tones, suggestive of a younger, potentially star-forming population, however, these regions are not very bright, indicating the presence of only minor star formation if any. There is no clear evidence of a spiral arm structure or significant dust lane obscuration visible at this resolution. The overall appearance points towards a galaxy that may be in a late stage of its evolution.
