The galaxy presents as a luminous elliptical, exhibiting a smooth, concentrated morphology. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population. Moving outward from the core, the galaxy's luminosity gradually decreases. The outer regions appear less defined, transitioning into the background sky. There is a slight elongation to the galaxy's overall shape, indicative of a cigar-like form, rather than a perfect sphere. The disk-like presence is extremely subdued and not easily distinguished. There are no clear indications of spiral arms, active star formation regions, or significant dust lanes within the galaxy. The overall smooth appearance supports that this galaxy is likely not undergoing any major mergers or gravitational disturbances.
