The galaxy presents a primarily smooth morphology, with a high degree of central concentration. The light distribution suggests an elliptical or lenticular classification, displaying a relatively featureless profile without obvious spiral arms or a prominent disk. The central region exhibits a brighter, more intense glow, potentially indicating the presence of a significant bulge or active galactic nucleus. Fainter, bluer emissions are present within the galaxy, particularly surrounding the central bulge, which could be indicative of younger stellar populations and ongoing star formation activity. The overall color of the galaxy is slightly redder than the blue emissions, suggesting an older stellar population. No signs of significant tidal disturbances or major mergers are readily apparent, although there is a possible minor asymmetry in the light distribution.
