The galaxy presents as a moderately bright, elliptical-shaped object with a smooth, diffuse morphology. A dominant, concentrated central bulge is apparent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Fainter, more diffuse extensions of light emanate from the central region, gradually fading into the background. The overall structure appears relatively undisturbed, lacking prominent spiral arms or signs of recent major mergers. The color profile indicates a likely absence of significant ongoing star formation within the galaxy, with redder wavelengths dominating the light output. It exhibits a smooth feature, with a shape somewhere between round and cigar shaped. There is no clear sign of any major disturbance.
