The galaxy presents as a single, relatively concentrated object. The morphology appears largely smooth, lacking prominent spiral arms or other distinct features. The object exhibits a roughly elliptical shape, appearing more round than cigar-shaped. There is a possible slight asymmetry in the light distribution.

The core of the galaxy displays a bright, yellowish-white hue, suggesting a population of older stars. The outer regions show a faint, diffuse extension with a subtle color gradient, transitioning towards slightly redder tones. This suggests the possible presence of some star formation activity, though it appears minimal overall. There is no obvious evidence of ongoing mergers or major disturbances in its structure.
