The galaxy presents a generally elliptical morphology, appearing significantly longer than it is wide. The light distribution shows a strong concentration towards the center, suggesting a prominent bulge. While the image resolution is limited, the galaxy appears relatively smooth in texture, with no immediately obvious spiral arm structures or significant dust lanes visible. There is no apparent evidence of ongoing major merging activity or tidal features, though the possibility of minor disturbances cannot be entirely excluded. The galaxy exhibits a reddish color, implying a population of older stars and a relatively low rate of current star formation. The overall visual impression is of a mature galaxy transitioning to a passive, quiescent state.
