The galaxy presents a largely smooth morphology, appearing somewhat elliptical in shape, though not perfectly rounded. There is some evidence of internal structure, potentially indicative of a disk or faint spiral arms, though these features are subtle. The central region exhibits a higher concentration of luminosity. The galaxy's color suggests a moderate mix of stellar populations, with hints of both older, redder stars and younger, bluer stars. There is some possibility of minor tidal disturbances or ongoing interactions with a neighboring galaxy, based on some slight asymmetries in the outer regions, although these are not pronounced. Star formation activity appears to be present, but is relatively low.
