The galaxy appears to be a relatively smooth, elliptical type. It has a bright, concentrated central bulge that transitions smoothly into a fainter, more diffuse halo. The shape is elongated, with a cigar-like appearance rather than perfectly spherical. The galaxy appears to be isolated, with no immediately obvious signs of ongoing mergers or major tidal disturbances, although there might be a hint of a minor disturbance. The central region exhibits a yellow to yellowish-white hue, suggesting an older stellar population. Fainter, bluish colors are observed in the outer regions, possibly indicating some ongoing star formation. The estimated size appears to be moderate, neither excessively large nor compact.
