This galaxy presents as a moderately luminous elliptical or lenticular system with a smooth, centrally concentrated light distribution. The core exhibits a yellowish-orange hue, suggesting an older stellar population likely dominated by evolved stars. The outer regions appear fainter and exhibit a subtle, diffuse bluish component. The galaxy appears elongated, with a cigar-like shape. No obvious spiral arm structures or significant dust lanes are visible. There appears to be no major ongoing merging activity but there is a chance that this galaxy exhibits minor disturbances. The morphology is relatively smooth and regular. The redshift indicates that the galaxy is relatively distant. Overall, this galaxy seems to be a massive and relatively quiescent system.
