The galaxy presents as a relatively compact object. Its overall morphology appears smooth and largely featureless, with no prominent spiral arms or bar structures discernible at this resolution. The light distribution is concentrated towards the center, suggesting the presence of a significant bulge component. The galaxy exhibits a generally round shape, with a slight hint of elongation. There is a subtle color gradient, with the central regions appearing more yellow-orange, potentially indicating an older stellar population. The outer regions have a slightly bluer tinge, suggesting ongoing or recent star formation, although the overall rate appears low. There is no clear evidence of tidal tails or other signs of recent major mergers or interactions. The galaxy appears relatively undisturbed.
