The galaxy exhibits a somewhat elliptical morphology, appearing more rounded than elongated. Its core is characterized by a bright, concentrated luminosity, suggesting a high density of stars. There appears to be a smooth transition from the core to the outer regions, with no distinct features or structures immediately apparent, though some slight visual disturbance is detected. A subtle blue tint is observed in the outer disk regions, possibly indicative of ongoing star formation. Overall, the galaxy presents a relatively quiescent appearance, lacking prominent spiral arms or significant dust lanes.
