The galaxy presents a smooth, elliptical morphology, characterized by a concentrated central bulge. The light profile transitions gradually from a bright, nearly circular core to a fainter, more diffuse halo. There is a hint of a very faint disk. The overall color index suggests a galaxy composed primarily of an older stellar population. Subtle color gradients may exist within the galaxy, with the central region appearing slightly redder than the outer regions. There is no evidence of significant dust lanes, spiral arms, or tidal features, suggesting a dynamically relaxed system with no recent major merger events. The galaxy is exhibiting low levels of star formation.
