The galaxy presents a generally smooth morphology, with a primarily spheroidal appearance. Its shape is somewhat elongated. A concentration of light emanates from the central region, decreasing radially outwards, suggesting a higher density of stars in the core. The galaxy's color index indicates it is a system dominated by an older stellar population, with some evidence of ongoing, though possibly subdued, star formation. There's no significant indication of dust lanes or prominent spiral arm structures. There do not appear to be signs of any major gravitational disturbance or ongoing merger events.
