The galaxy presents as an elliptical morphology, elongated in shape. The core region exhibits a strong concentration of light, appearing nearly uniform in color and suggesting an older stellar population. Moving outward from the core, the light intensity decreases gradually. The overall color profile is dominated by yellow, with a slight hint of red, suggestive of older stars and a lower rate of ongoing star formation. There is no visible evidence of spiral arms or significant dust lanes. Faint wisps of light extend beyond the main body of the galaxy, likely representing the outer halo of stars. The galaxy appears relatively undisturbed, lacking any obvious signs of a recent merger event or strong tidal interactions with other galaxies.
