The galaxy presents a generally elliptical morphology, appearing mostly smooth and with a high degree of central concentration. The light distribution suggests a prominent bulge component, characterized by a yellowish to reddish hue, likely indicative of an older stellar population. Surrounding the central bulge, a fainter, somewhat bluer disk component is marginally visible, exhibiting a less structured and more diffuse appearance. There are slight asymmetries that suggest that there might be some minor disturbances in the galaxy. The overall color profile leans towards the redder end of the spectrum, consistent with a mature stellar population and potentially a lower ongoing star formation rate.
