The galaxy presents as an elliptical morphology, exhibiting a smooth texture and a high degree of central concentration. It appears as an unresolved bright central core with a moderate degree of diffuse emission. The galaxy's light profile transitions smoothly from a compact core outwards, fading gradually into the background sky with slight elongation, neither perfectly round nor strongly cigar-shaped. There is no evidence of strong spiral arms or a distinct disk structure. The color indices suggest the galaxy is composed of an older stellar population. There are no visible signs of tidal tails, ongoing mergers, or major disturbances, indicating that the galaxy is in a relatively relaxed and undisturbed state. The object's intrinsic size appears to be moderate. The low star formation rate is consistent with a passive, early-type galaxy.
