The galaxy presents as a centrally concentrated, relatively smooth object. The overall color gradient transitions from a bright, yellowish core to a fainter, more greenish outer region. There is no discernible spiral arm structure. The galaxy's shape is generally round, without significant elongation. Faint extensions or tidal features are not apparent. The color profile suggests a population of older stars dominating the central region, while the outskirts may contain a younger stellar population. The light distribution is centrally peaked. There are hints of possible faint features along the edges of the galaxy. There is no evidence of dust lanes or active star formation. The galaxy appears to be relatively isolated, showing no signs of a major ongoing merger or significant tidal disruption. The smooth appearance indicates a possible elliptical or lenticular morphology.
