The galaxy presents as a relatively smooth, centralized concentration of light. Its morphology appears to be primarily spheroidal, exhibiting a lack of distinct spiral arm structures or a prominent disk. The light profile indicates a centrally concentrated brightness distribution that fades gradually outwards, indicating a relatively even distribution of stars. A slight elongation is visible, deviating from a perfectly circular form. There does not appear to be any major mergers or interactions with other galaxies. The galaxy appears to be relatively isolated within its immediate environment.
