This galaxy appears to be a relatively compact object with a smooth overall light distribution. It exhibits a near-spherical morphology, showing only a slight deviation from perfect roundness. Color gradients are present, with the central region appearing more yellow, suggesting an older stellar population and relatively low levels of ongoing star formation. The outer regions display a slightly bluer hue, indicative of a younger stellar population, though star formation activity seems subdued overall. There is no apparent evidence of spiral arms or other distinct features such as dust lanes or tidal tails, suggesting it is not currently undergoing a major merger or strong gravitational interaction.
