The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The core appears luminous with a yellow-white hue, indicative of an older stellar population. There is a noticeable decrease in surface brightness moving outward from the core, gradually fading into the background sky. The galaxy appears to be moderately rounded in shape, although the limited resolution makes it difficult to precisely define its ellipticity. No prominent spiral arms or distinct disk-like features are discernible. There is no strong evidence of ongoing major merger activity or significant tidal disturbances. Some faint, diffuse extensions are suspected, but these features are subtle. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy at a considerable distance, showing an evolved stellar population and a lack of significant star formation.
