The galaxy appears as a centrally concentrated, luminous object with a generally smooth morphology. The central region exhibits a bright, yellowish-white color, suggestive of an older stellar population. The galaxy does not show any obvious spiral arm structures or prominent dust lanes. There may be an extended, fainter halo surrounding the central core, but the transition is gradual. The overall shape is roughly circular, exhibiting only slight deviations from perfect roundness. There is no visual evidence of ongoing major mergers or significant tidal disturbances.
