The galaxy exhibits an overall elliptical morphology, appearing largely smooth and rounded. There is little evidence of spiral arm structure or significant disk features. The light distribution is centrally concentrated with a gradual decrease in brightness outward. Its color appears to be trending towards the redder end of the spectrum, with a mixture of green and yellow tinges in its central part. This suggests a stellar population dominated by older, redder stars, and reduced recent star formation activity. No major mergers or significant tidal disturbances are apparent. Close inspection reveals the absence of strong dust lanes.
