The galaxy presents a morphology that leans towards smooth and spheroidal in appearance. It exhibits an overall elongated shape, possibly cigar-shaped, rather than perfectly round. There is a notable absence of strong spiral arms or a well-defined disk structure. 

It is possible that this system is undergoing or has undergone a merging event. There appear to be some disturbances or irregularities in its overall structure and luminosity distribution, hinting at gravitational interactions. There is a secondary clump of increased luminosity to the right of the primary body which could be another galactic object. 

The color profile indicates a higher concentration of older stellar populations, with the redder hues dominating, suggesting relatively low ongoing star formation and a substantial mass. 
