The galaxy presents as a somewhat diffuse object, exhibiting a centrally concentrated luminosity profile. The primary morphology appears to be a spheroid, although subtle irregularities and possible faint extensions hint at potential past or ongoing interactions. The galaxy's color is generally consistent across its structure, with a slight redder tint in the central region, implying an older stellar population there. Given the disturbed morphology there is likely elevated star formation occurring in this galaxy, although more observations are needed to determine the nature of the disturbance. The overall impression is that of a galaxy undergoing some form of interaction or transformation, based on the overall luminosity and morphology.
