The galaxy presents as a somewhat elliptical, though predominantly rounded, form. The central bulge exhibits a high degree of luminosity, appearing almost uniformly bright across its extent. There is an observed radial decrease in surface brightness moving outward from the core. Hints of disk-like features are weakly suggested by subtle extensions of the galaxy's main body. Faint irregularities and possible disturbances in the outer regions may imply past interactions or ongoing minor mergers, although no clear tidal tails or prominent distortions are immediately apparent. The color profile suggests a relatively older stellar population, with a bias toward redder wavelengths, especially in the central region. Overall, the galaxy's morphology is consistent with an early-type spiral or potentially an elliptical galaxy with a small amount of ongoing star formation.
