The galaxy exhibits a moderately elliptical morphology, appearing somewhat elongated but not strongly cigar-shaped. It presents a centrally concentrated bulge region that transitions into a surrounding disk. The disk shows some indication of features or spiral arms.

The galaxy's color profile suggests a mix of stellar populations. The central bulge appears more yellowish-orange, implying an older stellar population. The outer disk regions show hints of bluer colors which may imply the presence of more recent star formation regions.

There are some irregularities within the galactic structure suggesting minor disturbances possibly caused by interactions. However, there is no conclusive evidence for major merging events or dramatic tidal features.
