The galaxy presents a primarily smooth morphology, with a slight elongation evident in its overall shape. The central bulge appears bright and concentrated, exhibiting a yellowish hue suggestive of an older stellar population. Emanating from the core are fainter, extended regions, which gradually fade into the background. There is a reddish region slightly offset from the core which may be the sign of an active star forming region. Overall, the galaxy shows little to no indications of strong spiral arms, and shows a light level that suggests it is a large, massive galaxy with suppressed star formation. There are signs of tidal disturbances or possible merger activity.
