The galaxy presents an ambiguous morphology. Its overall structure appears relatively compact and small. There is a suggestion of a central bulge, although it is not particularly prominent. A faint, somewhat indistinct disk may be present, but a clear disk-like structure is not definitively observable. No obvious spiral arms or bar structures are discernible. The overall light distribution is not uniform, showing some irregularity. There is a slight hint of possible tidal features or minor disturbances in the outskirts of the galaxy, which could suggest past interactions or a merger event. The color profile shows a slight concentration of redder hues in the central regions, with bluer colors appearing more dispersed in the outer regions. The redder core may indicate older stellar populations, while the bluer outskirts could be regions of more recent star formation. A more in-depth analysis, with consideration of additional data, is warranted to determine the precise nature and evolutionary history of this galaxy.
