The galaxy presents as a relatively smooth, elliptical morphology with a bright, concentrated central bulge. The light distribution appears fairly uniform across the galaxy, with a gentle decrease in intensity from the center outwards. There is little evidence of spiral arms or distinct star-forming regions. The color profile suggests a population of older stars, as indicated by the yellowish-red hue. No significant tidal features or signs of recent merger activity are apparent. The shape is close to circular. Overall, the galaxy appears to be a well-formed, evolved system.
