The galaxy appears as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated light profile, indicative of a significant stellar density, possibly an older stellar population. The galaxy's color appears to be mostly a pale yellow or white hue, suggesting the presence of evolved stars and a lack of significant ongoing star formation. The outer regions of the galaxy appear to fade gradually into the background, with little evidence of distinct spiral arms or features. There might be some minor disturbance in the galaxy, but it appears to be a single system. The round shape is elongated, but not extremely so. There does not appear to be evidence of a recent major merger.
