The galaxy presents a generally elliptical morphology, although some distortion is visible in its shape, appearing slightly elongated. The central region exhibits a bright, concentrated core suggesting a substantial concentration of stars. The inner region of the galaxy displays a yellowish-white hue, indicative of an older stellar population. Fainter, bluer regions extending from the core imply ongoing star formation. These blue regions seem to follow what may be faint, ill-defined spiral arm structures. However, the spiral pattern is not prominent. Overall, the galaxy appears relatively smooth with some indication of minor disturbances, but is not undergoing any major merger activity.
