The galaxy appears as a slightly elongated, faint source. The central region exhibits a brighter, more condensed luminosity. Extending outwards from this central condensation, there is a subtle, diffuse glow, suggesting the presence of a galactic disk. The color of the galaxy appears to be generally greenish. There are faint structures visible within the disk, implying some level of irregularity, potentially indicative of minor disturbances or interactions. The overall impression is of a relatively undisturbed galaxy with a moderately smooth morphology, yet with subtle hints of ongoing processes. The overall light profile seems to extend beyond the immediate bright core, indicating a non-negligible spatial extent. The overall faintness suggests it is relatively distant.
