The galaxy presents as a fairly smooth, elliptical morphology. It is observed to be elongated, with the major axis extending approximately twice the length of the minor axis. The central bulge region is bright and concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. This contrasts with the outer regions of the galaxy, where the light appears more diffuse and slightly redder. There is no discernible evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major merger activity. The overall color profile indicates a mature system with limited ongoing star formation.
