This galaxy presents as an elliptical morphology with a high degree of central concentration. The light distribution appears smooth and centrally condensed, with no evidence of spiral arms or a distinct disk component. The galaxy's shape is noticeably elongated, appearing cigar-shaped, with the major axis significantly larger than the minor axis. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population and reduced star formation activity compared to regions with a blueish tint. There are faint, diffuse extensions or halos surrounding the central bulge, though they are relatively indistinct. Overall, there is no indication of significant ongoing mergers or major disturbances.
