The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution suggests a higher stellar density in the core, with a gradual decrease in luminosity outwards. A slight elongation is discernible. There is minimal evidence of spiral arm structure or significant dust lanes, supporting a classification towards the early-type end of the Hubble sequence. There appears to be a general yellow/red hue with a hint of star formation.
