The galaxy presents as a somewhat diffuse and centrally concentrated object. Its overall shape is generally round, with slight deviations suggesting it is not perfectly spherical. There appears to be a central, brighter region, potentially indicative of a bulge. The color profile seems to shift from bluer hues in its outer regions to redder tones closer to its core. There may be some signs of minor disturbances within the galaxy's structure. A possible interaction is happening, or is in the recent past, given its possible merger morphology. Given these color properties and structure, a plausible interpretation points towards a significant, yet low, rate of recent star formation.
