The galaxy presents a relatively smooth, elliptical morphology, exhibiting a high degree of circularity. There's a discernible lack of prominent spiral arm structures or significant irregular features. The galaxy's light profile appears centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. No major mergers or tidal disturbances are readily apparent, although a subtle asymmetry or minor perturbation cannot be entirely ruled out upon further, more in-depth analysis. The overall color of the galaxy appears somewhat redder, indicative of an older stellar population and potentially lower ongoing star formation activity. The estimated size suggests it is a moderately sized galaxy.
