The galaxy presents as a single, relatively smooth structure. Its light profile is centrally concentrated with a diffuse, extended halo. The core exhibits a yellowish-white hue, which gradually transitions to redder tones in the outer regions. There is no discernible spiral structure or obvious dust lanes, suggesting a classification toward the elliptical end of the Hubble sequence. The overall round morphology implies a lack of significant rotational support, further supporting this conclusion. There is little evidence of recent or ongoing major merger activity, although the presence of minor disturbances cannot be entirely ruled out based on the present image alone. The galaxy's low specific star formation rate suggests a relatively quiescent stellar population with minimal active star formation. The estimated size is approximately 4 kiloparsecs in radius. The overall appearance is consistent with a mature elliptical galaxy at a redshift of approximately 0.18.
