The galaxy presents as a relatively compact object, approximately elliptical in shape, though there is a suggestion of slight elongation. Its morphology is generally smooth, lacking any immediately obvious spiral arm structures or significant dust lanes. The central region appears more luminous and concentrated, indicating a likely bulge component. There is a faint suggestion of a disk structure surrounding the bulge, based on its slight extension beyond the core. The galaxy appears to be a bluish-white hue overall, which tentatively indicates the presence of younger, hotter stars, but could also be affected by redshift. There does not appear to be evidence of any major ongoing merger activity or significant tidal disturbances in the immediate vicinity. The galaxy shows a degree of overall symmetry.
