The galaxy presents a generally smooth morphology, with a dominant central bulge exhibiting a yellowish hue, suggesting an older stellar population. The galaxy's overall shape appears to be somewhat elongated, deviating from a perfectly circular form. There is a subtle hint of disk-like structure, though it is not sharply defined. A minor disturbance is visible on one side of the galaxy, possibly indicative of a tidal interaction or past merger event. The object appears to be in the process of merging or gravitationally interacting with another galactic object, as evidenced by the distorted morphology of the disk and the presence of asymmetrical light distribution. The faintness of the outer regions suggests a relatively low rate of current star formation activity.
