The galaxy presents as a somewhat rounded, yet indistinct, elliptical-like structure. The central bulge exhibits a bright, concentrated luminosity, indicative of a high stellar density, and possibly an active galactic nucleus. The light profile appears to fade smoothly outwards from the core, with no prominent spiral arms or well-defined features easily discernible. There's a slight extension or asymmetry that might suggest minor tidal interaction or an internal disturbance. The overall color is relatively red, with only slight color variation across its structure, which may suggest an older stellar population, a relatively low star formation rate, and significant dust content.
