The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. A slight elongation is visible, but it generally appears rounded, though not perfectly so. The galaxy exhibits a radial gradient in luminosity, with the core region being significantly brighter than the outer regions. There are some subtle color variations present. The central bulge appears yellower, suggesting an older stellar population, while the outer regions exhibit hints of bluer hues, indicating the presence of younger, hotter stars. These bluer regions seem somewhat localized, suggesting potential pockets of star formation. There is no strong evidence of spiral arm structure or a prominent disk. No obvious signs of a major merger are apparent, though a minor disturbance or interaction cannot be ruled out, especially considering the slight asymmetry in the distribution of the bluer regions.
