The galaxy presents an elliptical morphology with a concentrated central bulge. The light distribution appears smooth and relatively featureless, lacking discernible spiral arms or a prominent disk structure. The color profile suggests an older stellar population, dominated by redder hues. There is a slight elongation in its shape, but it primarily exhibits a spheroidal form. No significant tidal disturbances or signs of ongoing major mergers are apparent. The galaxy appears relatively isolated with no nearby interacting companions. Overall, it appears to be a moderately massive system undergoing a relatively low rate of star formation.
