The galaxy presents as a relatively smooth, elliptical-like structure, though not perfectly symmetrical. There's a slight elongation to its form, appearing more lens-shaped than perfectly spherical. The central region of the galaxy exhibits a brighter concentration of light, possibly indicating a dense stellar population or an active galactic nucleus. Fainter, diffuse light extends outward from this central region. There appears to be a slight color gradient, with the central areas showing hints of yellow or orange, while the outer regions may exhibit a faint bluish tinge. This could suggest differences in the age or composition of the stellar populations within the galaxy, with older, redder stars dominating the core and younger, bluer stars possibly residing in the outer regions. The galaxy shows some indications of disturbance, but no apparent major merger features.
