The galaxy presents as a moderately bright, somewhat diffuse, oval-shaped structure. The central region exhibits a higher concentration of luminosity, appearing almost spheroidal. The color profile suggests a bluer hue in the outer regions, possibly indicating ongoing or recent star formation. There are hints of subtle disturbances or irregularities in its morphology, but no major signs of tidal tails or ongoing mergers are readily apparent, though minor disturbances cannot be ruled out. The galaxy does not appear perfectly round but rather somewhere between a round and elongated shape. It seems to be neither a pure elliptical nor a well-defined spiral galaxy, hinting at a possible transitional type or a lenticular galaxy with a weak disk component.
