The galaxy presents as a single, relatively smooth, centralized concentration of light. Its overall shape appears to be somewhere between round and elongated, possibly slightly cigar-shaped. While generally smooth, a subtle irregularity is discernible, hinting at a minor disturbance or perhaps the initial stages of a merger event. A central bulge is readily apparent. The color distribution is fairly uniform, showing no significant variations in stellar population across the galaxy's structure. Based on color, it appears to be a relatively active galaxy with ongoing star formation. 
