The galaxy presents as a somewhat regular elliptical, exhibiting a smooth light distribution across its structure. A concentrated bulge is clearly visible at the galaxy's center, appearing more luminous and with a redder hue compared to the outer regions. There are suggestions of a faint, diffuse disk surrounding the bulge, though the overall light profile indicates a morphology that is not dominated by spiral arms or distinct features. Color gradients are subtle, with a general shift towards bluer tones in the more extended areas, possibly indicating some degree of ongoing, albeit low, star formation activity away from the nucleus. The galaxy's overall shape is not perfectly spherical, leaning towards a slightly elongated, cigar-like form. There's no obvious indication of major mergers or significant tidal disturbances in the immediate vicinity.
