The galaxy presents as a relatively bright, elongated structure with a moderately inclined disk. A distinct bulge is not immediately apparent.

The color profile suggests a range of stellar populations, with bluer regions possibly indicating ongoing star formation. The galaxy exhibits some degree of asymmetry and irregularity which may indicate it has experienced a recent interaction or merger. There appears to be a tidal tail or bridge of material, suggesting the interaction may be ongoing. The galaxy has two regions of increased brightness towards the center.
