The galaxy presents as a somewhat elliptical, centrally concentrated object. Its overall color appears yellowish-orange, suggesting a stellar population dominated by older, evolved stars. There's little evidence of distinct spiral arms or prominent dust lanes. The light distribution is relatively smooth, with a gradual decrease in brightness from the central core outwards. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or nearby companion galaxies that would indicate a recent merger event. It is likely that this galaxy is a relatively massive system, with correspondingly low specific star formation rate and no indications of actively merging. Based on its morphology and color, this galaxy may be classified as an elliptical galaxy, exhibiting properties of a quiescent stellar population. The galaxy presents as a system that is viewed relatively face on.
