The galaxy presents a generally smooth morphology. A central bulge is evident, exhibiting a concentrated luminosity gradient. The overall shape is elliptical, trending toward a somewhat rounded appearance rather than a highly elongated one. Faint, diffuse outer regions extend from the brighter core, with no clear evidence of spiral arm structures or significant dust lanes visible in this image. There are no signs of major mergers or strong tidal disturbances. Color gradients suggest a possible decline in star formation rate away from the central regions.
