The galaxy presents a complex morphology, exhibiting evidence of a potentially ongoing or recent merger event. Its overall structure appears disturbed, lacking a clear, defined shape typically associated with elliptical or spiral galaxies. The light distribution is uneven, with brighter, concentrated regions suggestive of multiple galactic cores or intense star-forming knots. The color profile tends toward the redder end of the spectrum, indicating a population dominated by older stars and potentially high dust content, which could obscure younger, bluer stellar populations. There are also apparent disturbances in the galaxy's shape, possibly indicative of tidal forces at play due to interaction with another galaxy. It is also relatively smooth in texture, which could be due to a lack of gas or dust, or that a merger event has smoothed it out.
