The galaxy presents an overall smooth morphology, appearing largely featureless with a dominant central bulge. The light distribution suggests an elliptical or lenticular galaxy type. The central region exhibits a concentration of light, gradually fading towards the outer edges. There is a subtle color gradient visible, with a slightly yellower, presumably older stellar population concentrated towards the center, and a bluer hue in the outskirts, potentially indicating regions of younger star formation, though these are not prominent. The isophotes appear to be mostly regular, showing little evidence of strong tidal interactions or recent merger activity. The general shape is moderately round, with a slight elongation that is more in between round and cigar shaped. There are no readily apparent spiral arms, bars, or dust lanes visible in this image. Evidence suggests a relatively low star formation rate.
