The galaxy presents as a centrally concentrated, largely featureless object. It exhibits a smooth, somewhat elliptical morphology, though approaching circular. There is a slight elongation, but no distinct spiral arms or bar are discernible in this imaging. The color profile suggests a relatively evolved stellar population, with the light being shifted towards the redder end of the spectrum. There is minimal evidence of ongoing star formation, consistent with a quiescent or passively evolving system. The galaxy appears relatively isolated, showing no signs of major tidal interactions or recent mergers with other galaxies, though there might be some minor disturbances visible. Overall, it appears to be a fairly massive system.
