The galaxy presents an elliptical morphology, exhibiting a smooth and largely featureless structure. Its shape appears slightly elongated, deviating marginally from perfect sphericity. The galaxy displays a radial color gradient, with a bright, yellowish core that suggests a high concentration of older stellar populations. Moving outward from the core, the galaxy's color transitions to a bluer hue, potentially indicative of younger stars or ongoing star formation in the outer regions. The overall luminosity profile is centrally concentrated, diminishing gradually towards the edges. Faint, subtle irregularities are potentially present, and hint at past interactions. These interactions are not drastic, but they suggest that this galaxy may have undergone minor mergers in its past.
