The galaxy presents as a moderately luminous system with a redshift of approximately 0.1. Morphologically, it exhibits a dominant, smooth spheroid component indicative of an elliptical galaxy, with some intermediate properties of being slightly more elongated than circular. A subtle disklike structure is present, appearing almost edge-on with a relatively thin profile. This disk feature exhibits a distinct color contrast to the central bulge, with a blue hue suggesting the presence of younger stellar populations. The redder surrounding emissions suggests older, more evolved stellar populations are present in the bulge. There is no clear evidence of significant ongoing major merging activity, though subtle signs of minor disturbances cannot be entirely ruled out. Judging by its apparent size and distance, it is a reasonably massive system. Overall, this galaxy appears as a well-formed system displaying a range of colors in an intermediate stage between a pure elliptical and a spiral galaxy. Its star formation rate is suppressed to low levels.
