The galaxy presents as a single, concentrated light source with a slightly elliptical morphology. The central region exhibits a bright, yellowish hue, suggestive of an older stellar population. Fainter, less distinct blue-ish regions extend outwards from the core, potentially indicating areas of more recent star formation, although their presence is subdued. There's no clear evidence of spiral arms or a distinct disk structure. The overall smooth appearance indicates a system that is likely relatively dynamically relaxed. We see no major signs of disruption or ongoing merger activity, although subtle disturbances cannot be entirely ruled out based on the image alone.
