The galaxy presents as a moderately compact object with a noticeable disk-like structure. The light profile appears brighter in the central region, fading outwards into a diffuse halo. There are indications of potential disturbances in the galaxy's morphology, with a slight asymmetry observed in the outer regions, which could be related to tidal interactions. A possible merging event cannot be ruled out. The galaxy has a relatively smooth texture, but shows distinct features, which point to either faint spiral arm structures or disturbances. Further investigation is needed to determine its precise morphological classification and the nature of any interactions.
