The galaxy presents an overall elliptical morphology, with a dominant, smooth central bulge. A faint, disklike structure is tentatively observed, oriented approximately horizontally across the image. The bulge exhibits a yellowish hue, suggestive of an older stellar population, with a concentrated central region. The disk appears bluer in color, indicating the presence of younger stars and regions of active star formation. Some minor disturbances appear to be present on the left side of the galaxy, such as faint plumes or tidal features that may be interacting with it. Overall, the galaxy appears relatively isolated, without any obvious major merging events.
