The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth and featureless morphology. The light distribution indicates a spheroid-dominated system, with a high degree of symmetry. The core region appears bright and yellowish, suggesting an older stellar population, while the outer regions show hints of a bluer hue, possibly indicating regions of recent star formation, albeit at a low rate. There is no apparent evidence of spiral arm structure or significant morphological disturbance, such as tidal tails or merging features. The overall shape is tending toward intermediate ellipticity, it is more elongated than perfectly round. The galaxy appears to be relatively isolated.
