The galaxy presents as an elongated structure with a moderately smooth appearance. There is an indication of a central concentration of light, but no distinct nucleus is readily apparent. A faint, extended arm-like feature is visible on one side, suggesting a possible tidal interaction or recent merger event. The overall color appears to be slightly redder than the background field, suggesting a population of older stars and potentially a lower rate of current star formation. The galaxy's shape is more akin to a flattened spheroid, rather than a well-defined disk or sphere. Some distortion and irregularity can be observed. The apparent size is relatively small, indicating a significant distance.
