The galaxy appears as a singular, relatively smooth structure. It presents an elliptical morphology with an approximate effective radius of 6.9 kpc. There is a slight elongation of the galaxy shape, though not significantly cigar-shaped. The overall color profile suggests a moderate amount of ongoing star formation. There is no visible evidence of strong tidal disturbances or ongoing major mergers with other galaxies. The central region exhibits a slightly enhanced luminosity suggesting a compact nucleus or active galactic nucleus.
