The galaxy presents an elliptical morphology, elongated along a northwest-southeast axis. The core region exhibits a bright, concentrated luminosity, likely indicative of a high stellar density and possibly an active galactic nucleus, though further spectral analysis would be necessary to confirm AGN activity. Moving outwards from the core, the luminosity gradually decreases, with a smoother, less defined structure. There is some apparent irregularity in the outer regions, with a hint of possible tidal features or interactions, but no clear signs of on-going major mergers, this galaxy appears relatively isolated. The galaxy exhibits a predominantly redder color profile, with a more pronounced concentration of bluer light towards the center. Overall, the galaxy's morphology suggests an older stellar population with a relatively low star formation rate, although a small amount of ongoing star formation near the center cannot be ruled out.
