The galaxy presents as a somewhat elliptical, relatively smooth object with a clear central bulge. The color profile suggests an older stellar population dominating the central region, indicated by the yellowish-orange hue. There's evidence of a disk, and a very slight bluer color at the end of the major axis, hinting at the presence of younger stars or ongoing star formation in the outer regions. There is no clear spiral structure. The isophotes appear relatively undisturbed, suggesting minimal interaction with other galaxies. Overall, the galaxy appears to be a moderately luminous, fairly massive system experiencing a low rate of star formation.
