The galaxy presents as a largely featureless elliptical structure with a concentrated central bulge. The light distribution appears smooth and centrally condensed, exhibiting a radial decline in luminosity from the core outward. A slight elongation is observed, but overall, the shape is predominantly round. There are no apparent spiral arms, dust lanes, or significant star-forming regions visible in this image. The galaxy possesses a yellowish-red hue, indicating an older stellar population and minimal ongoing star formation. There are no visual indications of a major merger event or significant tidal disturbances. The galaxy appears to be relatively isolated, without any companion galaxies or signs of interaction.
