The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish hue, suggesting a population of older, less active stars. Surrounding the bulge is a fainter, more diffuse halo, appearing bluish, potentially indicating some presence of younger, hotter stars or ongoing star formation, albeit at a modest rate. No distinct spiral arm structure is discernible, suggesting a later-type classification. The overall roundness of the galaxy indicates a lack of significant rotational support or major recent merger activity. There is no obvious evidence of tidal tails or other strong disturbances. The galaxy's redshift implies it is relatively distant, with the observed colors representing a mix of stellar populations and a slight redshift.
