The galaxy appears to be a relatively smooth, elliptical type. It exhibits a high degree of central concentration, with the light intensity gradually decreasing towards the outer edges. There is a slight elongation, deviating marginally from a perfect circular shape. No distinct spiral arms or bar structures are discernible. The color profile suggests a population of older stars, evidenced by the redder hues, with limited presence of bluer, younger stars which would be indicative of ongoing star formation. There is no obvious evidence of significant tidal interactions or recent merger events, although a slight asymmetry may suggest minor past disturbances. The overall morphology suggests an evolved system approaching quiescence in terms of star formation activity.
