The galaxy presents as a relatively compact, ellipsoidal structure. The central region exhibits a high degree of luminosity, indicating a concentrated stellar population or active galactic nucleus. Moving outward from the core, the light gradually diminishes. A faint, somewhat diffuse extension is observable, presenting a possible asymmetry or tidal feature. The overall color appears slightly redder, suggesting an older stellar population, and/or a higher proportion of dust obscuring bluer wavelengths. There is weak evidence of a possible spiral arm structure, or perhaps a tidal tail emanating from the galaxy, though this is not very well defined. There is no obvious ongoing intense star formation within the galaxy.
