The galaxy presents as a relatively smooth, elongated structure. Its central region exhibits a bright, concentrated luminosity, suggestive of a prominent galactic bulge. The overall color profile appears to be somewhat redder in the central regions, transitioning to bluer hues in the outer disk. This color gradient could indicate an older stellar population concentrated in the bulge, with younger, bluer stars forming in the disk. There is little evidence of strong spiral arm structure or significant dust lanes within the galaxy. The shape is elliptical in appearance, it is largely undisturbed, but some minor interactions are possible. Overall, the galaxy appears to be a reasonably well-defined elliptical or lenticular galaxy, possibly in a relatively quiescent stage of evolution with a relatively low rate of star formation.
