The galaxy appears to be a relatively luminous system at a considerable distance, exhibiting a complex morphology. The primary component presents as a somewhat smooth, elliptical structure, concentrated towards a bright, yellowish core. This central region is surrounded by a fainter, diffuse halo of bluer light.

A notable feature is the presence of a disturbed area that is relatively bright and reddish in color, possibly indicative of active star formation. This region is located along the edge of the elliptical structure. It may represent a tidal interaction or a minor merger event. The overall shape of the galaxy is somewhat distorted. This suggests an ongoing interaction or a recent merger. The presence of both old stellar populations in the core and possible younger, star-forming regions contributes to the galaxy's overall spectral energy distribution.
