The galaxy presents as a relatively compact object with a smooth, diffuse appearance. It appears largely spheroidal, exhibiting a high degree of radial symmetry. There is no evident spiral structure or pronounced disk component visible.

The galaxy's light is concentrated toward the center, with a gradual decrease in luminosity as radial distance increases. The color profile appears largely uniform across the galaxy, with a subtle color shift towards the redder end of the spectrum. The isophotes appear regular and undisturbed.

Based on these features, a classification as an elliptical galaxy is plausible, perhaps of type E4-E6 on the Hubble sequence. Further spectroscopic data would be required to verify its composition, age, and internal kinematics.
