The galaxy presents as a centrally concentrated, relatively smooth elliptical system. There is a marked absence of defined spiral arms or a prominent disk structure. The light distribution is concentrated towards the center, with a gradual decrease in luminosity moving outward. The galaxy exhibits a yellowish-orange hue. This color profile suggests an older stellar population with a suppressed rate of star formation. The morphology implies a classification as an elliptical galaxy, likely of type E0-E3 due to its observed roundness. There is no apparent active galactic nuclei (AGN) activity in the core based on visible signs. The galaxy appears to be isolated, showing no visual indications of a major merger or significant tidal disturbances.
