The galaxy presents as a moderately luminous, early-type spiral. It is slightly elongated, appearing somewhat cigar-shaped. The central bulge is prominent and smoothly blended with the surrounding disk. There is little evidence of active star formation regions; the overall color suggests an older stellar population. No major disturbances or tidal features are observed, suggesting the galaxy has not undergone a recent major merger event. A subtle, disk-like structure can be discerned, but its features are not sharply defined.
