The galaxy presents as a relatively smooth, lenticular-shaped object. There appears to be a central bulge, exhibiting a yellowish hue suggestive of an older stellar population. Fainter, bluish light extends outwards from the bulge along the galaxy's major axis, potentially indicating the presence of a disk component with ongoing or recent star formation. The galaxy is elongated, appearing approximately four times as long as it is wide. There is a hint of a slight warp or tidal feature, possibly a minor disturbance in the galaxy’s morphology, although this could also be due to image artifacts. The overall structure suggests a galaxy that may be transitioning from a spiral to an elliptical morphology, with a generally low star formation rate.
