The galaxy presents an overall smooth morphology, appearing as an elliptical or lenticular type. The central bulge exhibits a concentrated luminosity, with a slightly elongated, cigar-shaped structure. Colors appear redder in the core, suggesting an older stellar population and/or dust obscuration, transitioning to a bluer hue towards the outer regions, potentially indicative of ongoing or recent star formation. There is no apparent spiral arm structure or evidence of a strong bar feature. Faint features surrounding the galaxy hint at possible minor disturbances or tidal interactions.
