This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a generally round morphology. It lacks distinct spiral arms or a prominent disk structure. There may be hints of subtle features or faint disturbances, but the galaxy's overall structure is dominated by a smooth, spheroidal component. The light distribution suggests a concentration of stars toward the central region. The color profile indicates a redder hue overall, likely associated with an older stellar population and low ongoing star formation. There is no significant indication of a major ongoing merger.
