The galaxy presents as a somewhat elongated structure, with an overall smooth appearance, and the light distribution suggests a dominant spheroid component. The color profile indicates a centrally concentrated reddish-orange hue, potentially suggesting an older stellar population or significant dust obscuration within the central region. There also seems to be some bluer regions, indicative of on-going or recent star formation. There are also areas of redder color on the exterior of the main body. It is difficult to assess any clear spiral arm structure, but the slight asymmetry and the presence of different colors suggests possible disturbances, perhaps the remnants of a minor merger event or tidal interaction. Overall, the galaxy appears to be in an intermediate stage of evolution, possibly transitioning from a more active star-forming phase to a more quiescent, redder state.
