The galaxy presents as a relatively compact system. It exhibits an overall amorphous morphology, with a notable deviation from a smooth, elliptical profile. Evident disturbances in its structure suggest possible gravitational interactions. The central region displays a slightly brighter concentration of light, though no distinct nucleus is clearly resolved. Faint tidal features or plumes are possibly discernible, further supporting the presence of ongoing or recent merger activity. The colour profile indicates a population of stars that are actively forming, this is supported by the system's moderately blue-ish colour, which is more consistent with the presence of younger, hotter stars. The galaxy's intermediate size suggests it may be a smaller galaxy.
