This galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, though not perfectly circular, appearing slightly elongated. The light distribution suggests a dominant bulge component with little to no discernible spiral arm structure, which makes sense given that most users think it's either smooth or an intermediate shape. The color profile is notably redder, indicating an older stellar population and potentially suppressed star formation activity. There is no obvious evidence of any major merging activity or tidal disturbances, which is also what most users are reporting.
