This galaxy presents as an elliptical morphology, with a relatively smooth and concentrated central bulge that transitions into a fainter, more diffuse outer halo. The core exhibits a bright, yellowish-white hue, indicating a population of older stars. There is a slight elongation to the overall shape, with the major axis oriented approximately northeast to southwest. The outer regions appear mottled, possibly suggestive of dust lanes or unresolved stellar populations. There is some evidence of a faint extension of the galaxy's light in the southwestern direction, which could indicate tidal interactions or a past merger event. The galaxy's color gradient suggests a redder population in the bulge and a slightly bluer population in the outer regions, hinting at ongoing or recent star formation at the periphery.
