The galaxy presents as a singular, yet perturbed, system. Its overall form appears elliptical with an observed smoothness. There is a presence of a secondary object seemingly interacting with the main galaxy body, indicating a possible merger event is occurring. This merging component displays a defined luminosity and concentrated form. The color gradient is redder than the main body, suggesting a greater proportion of older stellar populations. Overall the luminosity is moderate, with a gradual fading towards the outer regions. The inner core displays concentrated luminosity. There is minimal evidence of spiral arm structures or active star forming regions within the main body. The overall system appears to be in a state of flux due to ongoing gravitational interactions.
