The galaxy presents a generally elliptical morphology, appearing largely smooth and lacking prominent spiral arms or a distinct central bar. The light distribution suggests a centrally concentrated brightness profile, with luminosity decreasing gradually outwards from the core. A subtle color gradient is observed, the central region exhibiting a slightly redder hue in contrast to the more diffuse, bluer outer regions. This may indicate a difference in stellar populations or dust content between the galactic core and its outer disk. The overall structure is consistent with that of an early-type galaxy, possibly an elliptical or lenticular type, exhibiting little to no evidence of ongoing major merger activity or significant star formation. There is a slight ellipticity to the overall shape, suggesting some degree of rotational support. The angular size indicates it is a fairly small galaxy.