The galaxy presents as a luminous, centralized object. It appears generally smooth in morphology, displaying an elliptical shape. The central region exhibits a concentrated core of intense luminosity, suggesting a high density of stars or potentially an active galactic nucleus. Proceeding outward from the core, the intensity of the light gradually decreases. The overall color profile reveals a subtle shift from a more red hue towards the outer regions, implying variations in stellar populations and dust content. There is no clear evidence of prominent spiral arms, bars, or significant tidal disturbances. The galaxy's shape is predominantly round, with little indication of an elongated or cigar-like form. There may be a minor perturbation or irregularity along one edge, possibly indicative of a weak interaction.
