The galaxy presents a primarily smooth, elliptical morphology. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. There is a slight elongation observed, not quite spherical but trending toward it, with no obvious disk structures or spiral arms visible. Its overall color profile leans towards the redder end of the spectrum, indicative of an older stellar population and/or significant dust obscuration. No major mergers or significant tidal disturbances appear to be visibly affecting the galaxy's shape. There might be a minor, subtle irregularity hinting at a potential minor interaction, but it is not definitively conclusive from this image alone.
