The galaxy presents as a roughly elliptical, flattened structure. The light profile appears somewhat diffuse, indicating a smooth distribution of stars. A reddish color gradient is visible along the major axis, possibly indicative of dust extinction or an older stellar population in the central region. Evidence of disturbance is present and potentially indicative of a minor merger or tidal interaction. This distortion contributes to an irregular morphology deviating from a perfect ellipse. The core appears somewhat brighter than the outer regions, but the concentration of light towards the center seems to be moderate. There is potentially a band of material running through the galaxy, obscuring the center region.
