The galaxy appears as a centrally concentrated, smooth object, exhibiting an elliptical morphology. The light profile is dominated by a bright, yellowish core, indicative of an older stellar population. There is a subtle decrease in surface brightness moving outward from the center, with a gradual transition towards the galaxy's outer regions. Faint, diffuse extensions are visible, with no clear evidence of spiral arm structure or significant dust lanes. There are subtle hints of bluer hues in the outskirts, which might suggest the presence of some younger stars, though the dominant color suggests a population where star formation is relatively quiescent. The galaxy seems undisturbed with no signs of a recent major merger or interaction. The apparent roundness suggests that it is likely an E0-E3 type elliptical galaxy.
