The galaxy presents as a relatively smooth, elliptical structure. The core region is brightly illuminated with a yellow-white hue, suggesting an older stellar population. The overall shape is elongated, exhibiting a cigar-like morphology. A slight color gradient appears to be present, with the central bulge showing a more pronounced yellow-white tone, which may signify a higher concentration of evolved stars. No distinct spiral arm structures are visible. There is no evidence of any major mergers or significant tidal disturbances. The galaxy seems to be isolated, without any apparent interacting companions.
