The galaxy presents as a predominantly smooth, centrally concentrated structure. Its overall morphology appears elliptical, exhibiting a high degree of roundness with minimal deviation towards a cigar-shaped elongation. There is no readily apparent spiral arm structure or prominent disk-like feature, suggesting a classification towards the earlier end of the Hubble sequence, likely an elliptical galaxy.

The galaxy exhibits a color gradient, with a central region displaying a slightly yellowish hue, potentially indicating a population of older, redder stars. The outer regions show bluer tones, implying the possibility of some ongoing, but likely very low, star formation. No significant signs of major disturbances, mergers, or tidal interactions are observed. The galaxy's form is consistent with a relatively quiescent, isolated system undergoing minimal recent interaction.
