The galaxy presents as a moderately luminous, relatively smooth object. Its morphology appears elliptical to lenticular, exhibiting a central bulge that transitions smoothly into a more diffuse halo. There is a slight elongation of the galaxy along what appears to be its major axis. The color profile suggests an older stellar population, with a yellow-orange hue concentrated in the central region, possibly indicative of a higher density of evolved stars. There is minimal evidence of distinct spiral arms or significant dust lanes. The overall structure suggests a system that has undergone significant dynamical relaxation, with limited ongoing star formation. Faint, diffuse extensions can be seen, but there is no apparent interaction or merger activity.
