The galaxy appears to be a relatively small, low-mass system. Its morphology is characterized by a generally smooth, somewhat round structure with a noticeable, yet faint blue tinge suggesting a lack of significant dust obscuration. The object displays a subtle, yet noticeable feature extending away from the primary body of the galaxy that has hints of disk-like structure, possibly indicating a minor tidal interaction or disturbance. Some asymmetry is apparent in the galaxy's overall shape, potentially indicative of a past or ongoing merger event. The faintness of the object may be suggestive of an older stellar population with little active star formation.
