The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outwards into a fainter, more extended halo. The color profile suggests an older stellar population, with a yellow-red hue dominating the galaxy's overall appearance. There is little evidence of significant spiral arm structure or prominent dust lanes. The isophotes appear generally round. No signs of ongoing major mergers are apparent, though there may be minor tidal disturbances based on the image. The absence of bright blue regions indicates a low rate of current star formation.
