This galaxy exhibits an overall elliptical morphology, with an apparent cigar shape elongation along its major axis. The light distribution suggests a relatively smooth profile, with a higher concentration of luminosity towards the galactic center. The color gradient indicates a possible redder core transitioning to slightly bluer outer regions, suggestive of older stellar populations dominating the central bulge and younger populations potentially residing in the more extended areas. There is the suggestion of minor disturbances present. The galaxy exhibits properties indicative of a quiescent star formation rate, with a notable amount of evolved stellar populations within the object.
