The galaxy presents as a relatively compact, elliptical-like object. Its morphology appears largely featureless and smooth, with no immediately discernible spiral arms or bar structures. The light is concentrated towards the center, suggesting a prominent bulge or nucleus. 

There is an apparent color gradient, with a yellowish to white core that possibly contains an older stellar population. The outer regions show a slight hint of bluer hues, which may indicate the presence of some younger, hotter stars or ongoing star formation, albeit at a low level. The galaxy appears to be somewhat rounded. No signs of tidal tails or significant morphological disturbances are evident, suggesting it is not currently undergoing a major merger event, although some minor irregularities in the outer regions cannot be ruled out. 
