The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, featureless morphology. There is a general absence of distinct spiral arms or prominent dust lanes. The light distribution is centrally concentrated, with a bright nucleus that fades gradually towards the outer regions. The shape appears to be moderately elongated, but not highly flattened or cigar-shaped. There is no visual evidence of ongoing major mergers or strong tidal disturbances impacting the overall structure. The central region shows a slightly yellower color profile, while the outer regions are slightly bluer, potentially indicating differences in stellar populations. Overall, it appears to be an evolved galaxy likely with a low rate of star formation.
