The galaxy presents an overall elongated morphology, appearing somewhat cigar-shaped. A central bulge is visible, brighter and more concentrated than the outer regions.  There is evidence of a possible disk-like structure. The color profile suggests a predominantly older stellar population in the bulge, indicated by the redder hues.  Hints of a bluer component, possibly regions of active star formation, are present in a band that could be part of the disk.  There is a slight asymmetrical feature suggesting possible past gravitational interaction. This feature appears near the central bulge as a red area. Further analysis with higher resolution imaging is required to investigate the source of this distortion.
