The galaxy presents a smooth, centrally concentrated morphology. It appears as a roughly elliptical form, with the light distribution gradually decreasing from a bright core to a fainter outer halo. There is a slight elongation visible, suggestive of an oblate spheroid shape, but it is not strongly cigar-shaped. No prominent spiral arms or dust lanes are observed. The color gradient exhibits a trend toward bluer hues in the outer regions and redder color in the central region. This galaxy exhibits an absolute magnitude indicating it is likely a luminous galaxy and the mass indicates it is a massive galaxy. A low level of star formation may be occurring within the galaxy. Evidence from morphology reports suggests it is an isolated galaxy, not undergoing any major merging events. Overall, the galaxy appears to be an evolved system.
