The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. A prominent, bright nucleus dominates the galaxy's core, surrounded by a diffuse halo of light that fades gradually into the background. The color profile suggests a population of older stars, giving it a redder hue, especially within the central bulge. Evident is a minor perturbation nearby, suggesting the presence of a possible tidal interaction or remnant of a minor merger event. The main body of the galaxy shows a relatively well-defined structure. There are no strong indicators of active star formation regions within the observed bands, suggesting a relatively quiescent state.
