The galaxy presents as a centrally concentrated, relatively smooth structure. It exhibits a generally elliptical morphology, appearing quite rounded in shape. There is a noticeable color gradient, with the central region displaying a yellowish hue, indicative of an older stellar population. The outer regions show a subtle transition towards bluer colors, suggesting the presence of younger, hotter stars, although this population is not dominant. There is no visible spiral structure or prominent dust lanes, implying a lack of significant ongoing star formation. The overall appearance is consistent with an early-type galaxy, likely an elliptical or lenticular galaxy, at an approximate distance where finer structural details are not easily resolved. There is no obvious evidence of a major merger event or significant tidal disturbances in its immediate vicinity.
