The galaxy presents as a centrally concentrated, elliptical system, generally smooth in appearance. The color gradient shifts slightly towards redder hues in the central regions. No obvious spiral arm structure or distinct dust lanes are visible. The galaxy appears relatively undisturbed, showing no strong signs of ongoing major merger activity or significant tidal interactions. There might be a very faint extension of light surrounding the main body of the galaxy, which could potentially be a stellar halo or diffuse envelope. The overall morphology suggests a relatively evolved galaxy, likely with a substantial population of older stars. The relatively smooth light distribution is consistent with a high degree of rotational symmetry.
