This galaxy presents as a moderately luminous object with an elongated, cigar-like morphology. Its color profile suggests a composition of older stellar populations. The presence of a smoother texture indicates a higher fraction of evolved stars, likely dominating the overall light emission. There is a hint of a weak disk-like feature. It does not obviously appear to be undergoing any major merging events or significant disturbances, suggesting a relatively quiescent state. Although the primary light is redder, there is a hint of blue regions near its center. This could mean ongoing star formation, though on a small scale compared to its overall mass.
