The galaxy presents as a centrally concentrated, elliptical-like object with a smooth, featureless morphology. The core region exhibits a distinct yellowish-orange hue, suggesting a population dominated by older stars. The galaxy displays a relatively high degree of roundness. There is no apparent spiral structure, bar, or evidence of recent or ongoing major mergers or tidal disturbances. Faint blue fringes can be detected at the edges of the galaxy, indicating the presence of some younger, hotter stars, although their number appears to be small. The color gradient from the center to the edges suggests a decline in the mean stellar age with increasing distance from the core. Overall, the galaxy seems to be an evolved system with a modest amount of recent star formation.
