The galaxy presents as a relatively smooth elliptical or lenticular system, exhibiting a moderate degree of roundness in its overall morphology. There is subtle evidence of a possible interaction or disturbance in its structure, hinting at either a minor gravitational influence or a past merger event. The galaxy displays a concentration of light that is slightly more intense towards its core, with a gradual decline in brightness moving outward. Color gradients suggest a population of older stars, as indicated by the redder hues within the central regions. There is also bluer light in the tidal features that suggests younger stars may be forming in these regions. The galaxy shows no strong indication of spiral arm structures or prominent dust lanes. Overall, this galaxy appears to be a quiescent system.
