The galaxy appears as a singular, relatively smooth structure. The morphology suggests a predominantly elliptical galaxy type, evidenced by its round appearance and lack of discernible spiral arms or a prominent disk. The light distribution is centrally concentrated, with a bright core that gradually fades towards the edges of the galaxy. The color profile indicates a galaxy dominated by older stellar populations, exhibiting a yellowish-red hue across its entirety, indicative of lower star formation rates and the presence of evolved stars. There is no clear evidence of recent or ongoing major merging activity or significant tidal disturbances; the object appears relatively undisturbed and relaxed. The galaxy’s radial profile suggests a fairly smooth light distribution, lacking bright knots or HII regions that would denote areas of active star formation.
