The galaxy presents a smooth, largely featureless appearance. It exhibits an elliptical morphology, with a slight elongation. The light distribution is centrally concentrated, with brightness decreasing gradually outwards. The galaxy has a somewhat round shape, with an axis ratio approaching unity. Colors appear consistent with an older stellar population, with a tendency towards redder hues. There is no clear evidence of spiral arms or significant dust lanes in the image. There is very little indication of recent or ongoing major merger activity, though there is some minor disturbance that cannot be easily characterized based on this image alone. The galaxy's light profile appears consistent with a Sersic profile, indicating a bulge-dominated structure.
