The galaxy presents a distinct, elongated morphology. There appears to be a primary central bulge, exhibiting a smooth, concentrated distribution of stellar light. This central region displays a yellowish-orange hue, possibly indicative of an older stellar population.

A secondary, smaller concentration of light is also present, potentially a secondary bulge. The galaxy exhibits a notable degree of disturbance or interaction, as suggested by the irregular shape and the presence of two concentrations of light. There are no clear spiral arm structures visible. The overall color suggests intermediate levels of recent star formation activity.

