The galaxy presents as a moderately inclined disk system. The central bulge appears significant, exhibiting a yellowish hue suggestive of an older stellar population. Moving outward from the bulge, a bluer disk is discernible, hinting at regions of ongoing star formation. The overall structure is relatively smooth, though some subtle irregularities in the outer disk might indicate minor gravitational interactions or internal disturbances. The galaxy's morphology suggests a transition between an elliptical and a spiral galaxy, likely an early-type spiral with a dominant bulge. The disk is not strongly defined, and spiral arms are not clearly visible. The galaxy exhibits a moderate redshift, implying a considerable distance and lookback time.
