The galaxy exhibits a somewhat amorphous structure, lacking a distinct spiral or elliptical form. It presents as a collection of luminous clumps embedded within a fainter, more diffuse halo or envelope. These clumps vary in color, with some appearing a yellowish-orange hue and others exhibiting a bluer tint. The overall luminosity profile is complex, showing no clear central concentration. There is evidence of possible tidal features or distortions, particularly around the periphery of the galaxy, suggesting a potential interaction or merger event. The galaxy's shape is not perfectly round. The redder clumps may indicate regions of older stellar populations or dust obscuration, while the bluer regions likely contain younger, hotter stars.
