The galaxy presents as a moderately luminous object with an elliptical morphology. The light distribution appears relatively smooth, with a concentrated central bulge and a gradual falloff in surface brightness towards the outer regions. There is a slight elongation in its shape, departing from a perfectly circular profile, appearing more cigar shaped. There is a lack of any distinct spiral arm structure or prominent dust lanes, suggesting that it is an elliptical galaxy. The galaxy exhibits a yellowish-red color indicative of an older stellar population and/or significant dust extinction. There is no visual evidence of ongoing major merger activity or strong tidal distortions. The galaxy displays a central, bright region, potentially indicating either a high concentration of stars or the presence of an active galactic nucleus (AGN). Overall, it seems that there has not been a lot of recent star formation.
