The galaxy presents a generally smooth morphology, appearing as a centrally concentrated elliptical or lenticular type. There is a high degree of central concentration with a bright core, indicating a substantial stellar population within the nuclear region. A flattened disk is not obviously present, though subtle variations in color and luminosity suggest possible features. The color distribution is not uniform, exhibiting a subtle reddening in the central regions, implying an older stellar population, and bluer hues in the outer regions. The overall shape appears largely regular, without significant signs of ongoing major mergers or tidal disruptions, though minor disturbances cannot be completely ruled out. The galaxy is relatively isolated in the image, with no immediately interacting companions. Based on these observations, the galaxy is consistent with a moderately massive system.
