The galaxy presents with a moderately bright central bulge, exhibiting a smooth, concentrated light profile. The surrounding disk structure is weakly defined, appearing somewhat amorphous and lacking distinct spiral arm features. The overall color suggests a relatively young stellar population, particularly in the central region, as evidenced by the blue-green hue. A faint, extended halo or tidal feature might be present, subtly encompassing the main body of the galaxy, indicating potential past interactions or ongoing accretion events. A slight asymmetry in the outer regions could further support this hypothesis. Based on the features, the galaxy appears to be in the early stages of merging with a smaller galaxy. 
