The galaxy presents a largely smooth, elliptical morphology. The central bulge is prominent, exhibiting a bright, concentrated luminosity with a yellowish hue. There is a gradual decrease in surface brightness moving outward from the core, with no readily apparent spiral arm structure. The galaxy appears generally isolated, without strong indications of ongoing tidal interactions or major mergers. There may be evidence of some minor disturbances within the galaxy, as indicated by slight irregularities in the outer isophotes. The shape is somewhat in between elliptical and circular. Star formation rate is low, suggesting an evolved stellar population. The galaxy is of significant mass, likely populated mostly by older stars.
