The galaxy presents as a somewhat diffuse object with a notable blue hue, indicative of ongoing star formation. The overall morphology appears disturbed, possibly exhibiting signs of an interaction or merger. The light distribution is uneven, suggesting the presence of distinct regions with varying stellar populations. While the central region is not clearly defined, there is a brighter, slightly more compact area offset from the apparent center, which may be a dense stellar cluster or active galactic nucleus. Faint extensions or tidal features seem to emerge from the main body, further supporting the interaction hypothesis. The galaxy's estimated size places it as a medium sized system.
