The galaxy presents as a moderately bright, slightly elongated, lenticular-like structure. There is a central bulge exhibiting a yellowish hue, suggesting an older stellar population concentrated in the core. Surrounding the bulge, a fainter, bluer disk component is visible. The outer regions of the disk appear somewhat irregular. The overall morphology suggests a galaxy that may be transitioning from a spiral structure to a more featureless elliptical form, potentially due to a past merger or ongoing interactions. A small portion of the galaxy is experiencing a minor disturbance. The lack of prominent spiral arms indicates a relatively quiescent state of star formation.
