The galaxy presents as two distinct components, likely interacting or merging. The dominant component appears relatively smooth and spheroidal, exhibiting a strong central concentration of light. Its color profile skews towards the blue end of the spectrum, suggesting a population of younger, hotter stars. This component is roughly circular in appearance.

The secondary component displays a more elongated, less defined structure. Its color is significantly redder than the primary component. There is a faint, ill-defined structure around this galaxy, suggesting some level of gravitational disturbance. Overall, the system does not appear to be undergoing a major, violent disruption but displays mild signs of possible tidal interaction.
