The galaxy presents a somewhat diffuse and asymmetrical morphology. The light distribution appears uneven across its extent. There is a slight concentration of light towards the center, but a defined nucleus is not clearly visible. Faint tidal tails or plume-like structures appear to emanate from the main body of the galaxy on one side. There's a hint of disturbance within the galaxy's structure, possibly indicative of a past or ongoing interaction or minor merger event. The color profile is dominated by redder tones, suggesting a population of older stars. The bluer component is relatively weak, implying limited ongoing star formation.
