The galaxy presents as a slightly elongated, lenticular-like structure. It exhibits a smooth, relatively featureless morphology with a subtle color gradient from the central region outwards. The central bulge appears slightly brighter and more concentrated. There is no strong evidence of prominent spiral arms or distinct dust lanes. The galaxy's overall color suggests a population of older stars, with a possible lack of significant ongoing star formation. There might be minor disturbances present, but the overall structure appears largely undisturbed, implying no major ongoing merger events. The estimated size suggests a substantial galaxy, possibly containing a large mass.
