The galaxy presents as a slightly elongated, lenticular or early-type spiral morphology. It exhibits a relatively smooth, centrally concentrated light distribution, indicative of an evolved stellar population. A subtle, reddish hue dominates the galaxy's color, suggesting a lack of significant ongoing star formation and a population of older, redder stars. The galaxy appears moderately large, with an estimated physical size around 10 kpc, and the overall structure implies a relatively high mass system. There is a potential hint of minor tidal disturbances or asymmetry in the outer regions, perhaps indicative of past or ongoing interactions, but the primary impression is that of a relaxed, well-defined galaxy. Integrated light indicates an absolute magnitude characteristic of bright galaxies at its redshift.
