The galaxy presents as an elongated structure, exhibiting a notable degree of asymmetry. One side of the galaxy appears more condensed and exhibits a yellowish-red hue, suggesting an older stellar population and/or significant dust obscuration. The opposing side displays a bluer tint, indicative of more recent star formation activity. A disk-like morphology is weakly suggested, though not clearly defined. There appears to be a minor disturbance, which could be due to interaction with a smaller galaxy, though it's not a clear merger. The galaxy appears relatively large. Overall, the galaxy presents with characteristics of a relatively massive system with low levels of star formation.
