The galaxy presents a largely smooth and centrally concentrated morphology. It exhibits a moderately elliptical shape, appearing neither perfectly spherical nor highly elongated. The color profile suggests a dominant population of older stars, as indicated by the redder hues concentrated towards the galactic center and less prominent blue star forming regions. The galaxy is generally undisturbed in its appearance, showing no obvious signs of recent major mergers or tidal interactions. A faint disk may be present, but further spectral analysis is needed to confirm. There is a low likelihood of significant on-going star formation.
