The galaxy appears as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge. There is a gradual decrease in light intensity moving outward from the center. The galaxy's color profile indicates a redder core region, suggesting an older stellar population dominated by evolved stars. The outer regions present a slightly bluer hue, hinting at a younger stellar population or possibly ongoing, low-level star formation, though this is not strongly apparent. There is no clear evidence of spiral arm structures or significant dust lanes. The overall morphology suggests a galaxy that is likely to be in a relatively late stage of its evolutionary history. The galaxy does not appear to be undergoing any major mergers or tidal interactions. There is some asymmetry, but it's subtle and could be due to internal dynamics or minor past interactions.
