The galaxy presents as a luminous elliptical, with a smooth, centrally concentrated profile. The overall color is a yellow-red hue, suggestive of an older stellar population. There is no distinct spiral arm structure or prominent dust lane visible. The galaxy appears relatively undisturbed, exhibiting no obvious signs of a recent major merger, though a very minor disturbance is possible. It has a generally rounded shape, without a highly elongated or cigar-like morphology. The light distribution fades gradually from the core outwards. The overall appearance suggests a relatively massive system with a low star formation rate.