The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical, with a noticeable elongation along one axis. There is a bright central bulge that gradually fades into a less luminous halo or disk component. The color gradient suggests a higher concentration of older stellar populations in the central region, which exhibits a yellowish hue, possibly indicative of a lack of significant ongoing star formation in that area. The outer regions show a slightly bluer tinge which may indicate the presence of some younger stars or star forming regions, but no distinct spiral arms or other prominent features are evident. There's no visually apparent tidal disruption or other sign of recent interactions with other galaxies, suggesting relative isolation.
