The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology, with a high degree of roundness. There is no apparent evidence of a prominent disk structure, spiral arms, or bar feature. The galaxy's color appears yellowish-orange, suggesting an older stellar population with relatively low ongoing star formation. There is no readily apparent indication of a major merger or strong tidal disturbance; however, there is some indication of a minor irregularity in the outer regions.
