The galaxy presents as a singular, relatively smooth object with a concentrated central region exhibiting a yellow-white hue, suggestive of an older stellar population. Fainter, diffuse extensions radiate outwards from this core. There appears to be a slight asymmetry in the distribution of light, with a hint of redder tones visible on one side, potentially indicating regions of dust obscuration or areas of more recent, albeit subdued, star formation activity. There is evidence this galaxy may be undergoing a merging event.
