The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless light distribution. The core region displays a higher surface brightness, gradually decreasing towards the outer edges. The galaxy appears round. There is no apparent dust lane, spiral arm structure, or significant tidal disturbance visible in the image. The color profile suggests a population of older stars, indicated by the redder hue. The galaxy does not appear to be actively undergoing any major merging events, as evidenced by the lack of significant morphological distortions. The overall appearance is consistent with an evolved system with a low star formation rate.
