The galaxy presents as an elongated, somewhat disturbed system. The central region appears smooth, with a bright, concentrated core exhibiting a slight pinkish hue. Emanating outwards from the core is a bluer, more diffuse glow. The galaxy's overall shape is intermediate between round and cigar-shaped. There appears to be ongoing or recent merger activity or tidal interaction, resulting in some irregularities in the galaxy's outer structure. While a substantial fraction of the galaxy is smooth, there is also evidence of a disturbed disk. Star formation is present, and the stellar mass is estimated to be substantial.
