The galaxy presents a generally elliptical morphology, appearing more elongated than circular. The luminosity profile suggests a concentrated central bulge that diminishes gradually towards the outer regions. Color gradients are subtle, but there is a faint indication of bluer hues in the outer regions, potentially indicative of more recent star formation in these areas. The overall color is relatively red, implying an older stellar population dominates. No distinct spiral arms or prominent dust lanes are visible. There is no visible evidence of a major ongoing merger event, though the possibility of minor tidal disturbances or past interactions can't be completely ruled out. The galaxy exhibits a smooth appearance overall, lacking detailed features, suggesting it may be a relatively quiescent system.
