The galaxy presents as a relatively smooth, elliptical-like object, though some slight irregularities are visible upon closer inspection. It appears to be a concentrated structure with a bright central bulge that gradually fades outward into a less defined halo. The color profile suggests an aging stellar population, leaning towards yellow. Faint hints of bluer regions are present, possibly indicating pockets of younger stars or ongoing star formation, though these are not prominent. There is a subtle suggestion of a disk component, but the overall structure is dominated by its spheroidal shape. No significant dust lanes or spiral arm structures are apparent within this image. It appears to be relatively isolated. There are no indications of recent or ongoing major merger activity.
