The galaxy appears as a moderately bright, lenticular object with a redshift of approximately 0.13. The galaxy is roughly elliptical in shape, though exhibiting characteristics of an intermediate disk galaxy. A significant portion of the galaxy's light is concentrated in the central region, indicating a prominent bulge. There appears to be evidence of faint disk-like structures extending from the central bulge. The colors suggest a range of stellar populations. The central bulge exhibits a yellow-orange hue, suggesting an older stellar population. The outer disk appears slightly bluer, implying more recent star formation activity. There is a possibility of minor disturbances within the galactic structure, though no major mergers or violent interactions are immediately apparent. The overall morphology appears relatively undisturbed, suggesting a galaxy in a later stage of its evolution with a moderate stellar mass and low star-formation rate.
