The galaxy presents as a relatively smooth, centrally concentrated object. It appears largely featureless, lacking any obvious spiral arms or bar structures. The light profile indicates a significant bulge component, with the luminosity peaking towards the center and gradually fading outwards. The color gradient is subtle, with a slightly bluer hue in the outer regions compared to the more yellow/red core. This could indicate ongoing star formation in the outskirts, while the core is dominated by an older stellar population. The overall rounded shape suggests a classification towards the elliptical end of the Hubble sequence, but the slight bluing hints at the possibility of a disk component or a recent minor merger event. There is no clear sign of any major disturbances or tidal features associated with a recent major merger. Overall, it appears to be a galaxy of intermediate mass with a moderate rate of star formation.
