The galaxy presents a somewhat elliptical morphology, appearing generally smooth and featureless at this resolution. The light distribution suggests a centrally concentrated structure, with a gradual decrease in luminosity towards the outer regions. Its color profile indicates a redder hue overall, which potentially suggests an older stellar population and/or significant dust obscuration. However, there are subtle hints of bluer components that might indicate some ongoing, but low, level of star formation activity. There seems to be ongoing tidal interactions or a past merger event, due to faint surrounding dust or matter, but more detailed analysis is needed to determine merger classification.
