The galaxy appears as a relatively smooth and elliptical structure, with a concentrated central bulge. Its light profile suggests a high Sersic index, indicating a centrally concentrated luminosity distribution. There is no visible evidence of spiral arms or strong disk features. The galaxy exhibits a slight elongation, and its overall shape appears close to round. The color is somewhat redder, indicating a more evolved stellar population and a suppression of star formation activity. No significant tidal features or signs of recent major mergers are apparent. The galaxy shows little evidence of internal dust extinction. Overall, it is categorized as an early-type galaxy with a relatively smooth morphology, evolved stellar population, and minimal ongoing star formation.
