The galaxy presents a generally elliptical morphology, appearing largely smooth and spheroidal in shape. Its core exhibits a high surface brightness, with a concentrated luminosity gradient towards the central region. Color analysis reveals a dominant yellow-red hue, suggestive of an older stellar population and a relative lack of active star formation within the galaxy's core.

The outskirts of the galaxy display a fainter, more diffuse luminosity, fading into the background sky. There is a subtle hint of a disk-like structure, but the galaxy's round appearance suggests that it is likely an elliptical or lenticular galaxy rather than a spiral. There are no prominent dust lanes or spiral arms visible in this image. There appears to be a slight disturbance to the upper right of the core.
