The galaxy presents as a slightly elongated, elliptical form, appearing relatively smooth in texture. A central bulge is evident, exhibiting a concentrated luminosity, with color tending towards the yellow/orange spectrum. The luminosity gradually diminishes outwards from the central region, lacking distinct spiral arm structures or prominent dust lanes. The galaxy appears to be fairly isolated, showing no immediate signs of tidal interactions or major mergers, although subtle distortions cannot be entirely ruled out. The overall color suggests a stellar population dominated by older, redder stars, with a possibly suppressed rate of ongoing star formation. The absence of significant blue light further supports a lack of abundant young, massive stars. The galaxy's moderate size and somewhat diffuse outer regions indicate it is likely a galaxy of intermediate mass.
