The galaxy presents a somewhat amorphous morphology. The light distribution appears fairly smooth, with a bright, concentrated core region. There are no obvious spiral arm structures or a well-defined disk component. Faint, extended features or tidal tails do not appear to be prominent, though there is a hint of minor asymmetry in the outer regions. The galaxy's color profile indicates a relatively blue hue, suggestive of ongoing or recent star formation activity, particularly in the central regions. The relative lack of redder colors might indicate a lower abundance of older stellar populations or dust obscuration. There is a possible interaction with another object, or some merger-like event that has previously taken place. 
