The galaxy presents as a moderately luminous object with an apparent smooth morphology. The light distribution suggests a centralized concentration, indicative of a prominent bulge. There may be a faint disk component. The galaxy appears to be undergoing a possible merging event or interaction, evidenced by the presence of a secondary component located relatively close to the central galaxy, or a tidal disturbance in the main galaxy. The color profile indicates a reddish hue, potentially suggesting an older stellar population.
