The galaxy presents as a diffuse, somewhat elliptical object. Its core exhibits a concentrated luminosity, appearing a warm yellow-orange hue, suggestive of an older stellar population. The outer regions of the galaxy gradually fade into a fainter, more indistinct halo. A slight asymmetry is discernible, with a hint of what could be a minor disturbance or a very faint spiral arm structure. Overall, the galaxy seems to be relatively smooth, with no prominent signs of significant star formation or recent major merger events. The color profile points to a relatively low star formation rate.
