The galaxy presents as a smooth, elongated structure, suggestive of an elliptical morphology. A concentrated central bulge is discernible, with light gradually fading towards the outer edges. The color profile is dominated by yellow and red hues, implying a population of older stars, characteristic of elliptical galaxies with low star formation rates. There may be a slight disk structure but it is not very clear. The light distribution is relatively even, lacking prominent spiral arms or distinct features associated with active star formation, further supporting an elliptical classification. There are no apparent signs of ongoing major mergers or significant tidal disturbances.
