The galaxy presents as a relatively compact object with a moderate spatial extent. The light profile appears to be centrally concentrated, suggesting a spheroidal morphology. The galaxy exhibits a smooth, diffuse appearance, with little evidence of spiral arms or prominent disk features. 

There appears to be some level of disturbance in the overall morphology, possibly due to a past or ongoing interaction. There may be a slight elongation or asymmetry in the outer regions of the galaxy. Based on the color indices and the general morphology, the galaxy's stellar population appears to be dominated by older stars, giving it a reddish hue. There is some indication of bluer regions, possibly indicating pockets of younger star formation, but these are relatively subdued.
