The galaxy presents as a relatively smooth, elliptical morphology with an apparent cigar-shaped structure. There is a concentrated central bulge that exhibits a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a fainter, more diffuse halo with subtle bluish tones, potentially indicating some younger, star-forming regions. No prominent spiral arms or dust lanes are discernible within the image, and there is no obvious evidence of major mergers or significant tidal disturbances. Minor asymmetrical distortions could indicate some potential gravitational interactions. The galaxy is overall fairly symmetrical.
