The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. It presents an elongated shape, with the major axis significantly longer than the minor axis. The core of the galaxy displays a concentrated luminosity, transitioning gradually to a less dense outer region. A slight color gradient is observable, with the central bulge tending toward a yellow/orange hue, potentially indicative of an older stellar population. The outer regions exhibit a bluer tint, possibly signifying regions of more recent star formation activity, although not very prominent. No distinct spiral arms or bar structures are discernible. There is no evident presence of ongoing major mergers or tidal disturbances; though, a possible faint asymmetry in the outer regions may indicate past interactions. The overall impression suggests a relatively massive galaxy.
