The galaxy presents as a roughly elliptical or lenticular structure with a concentrated central bulge. The light distribution appears smooth, without prominent spiral arms or distinct dust lanes visible in this image. There is a slight color gradient, with the central bulge exhibiting a yellowish hue, potentially indicating an older stellar population, while the outer regions show a bluer tint, suggestive of more recent or ongoing star formation activity. The overall morphology implies a system that may be in a relatively late stage of its evolution, with a reduced star formation rate compared to actively star-forming galaxies. There are no obvious signs of significant tidal interactions or mergers affecting the galaxy's overall structure; however, subtle disturbances may not be resolved at this resolution.
