The galaxy presents an elongated morphology, appearing significantly longer than it is wide. There is a clear central bulge, which is yellowish in color, suggesting an older stellar population. Extending from this bulge, a diffuse structure emanates, displaying a bluish hue which indicates the presence of younger, hotter stars. This extended structure is somewhat irregular, appearing less defined on one side compared to the other. There appears to be some disturbance in its morphology, with an asymmetry. Overall, this galaxy shows characteristics of a disk galaxy undergoing some form of disruption or tidal interaction.
