The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. The overall light distribution suggests a well-established stellar population, with a significant contribution from older, redder stars, especially concentrated toward the core. The apparent morphology does not show any obvious signs of spiral arms or prominent disk features. There might be some indications of minor tidal disturbances or interactions in the surrounding area, but the primary structure of the galaxy remains largely undisturbed. The galaxy appears to be somewhat compact, exhibiting a concentrated light profile.
