The galaxy appears as a moderately bright, somewhat symmetrical elliptical. Its core exhibits a noticeable concentration of light, fading gradually towards the outer edges. The color profile suggests a population of older stars, leaning towards redder wavelengths. No spiral arms or distinct features are immediately apparent, supporting the classification as elliptical. There's no apparent dust lane or signs of recent merger events. Its morphology suggests a relatively relaxed system, and a well-established spheroidal shape is observed. There may be a slight elongation of the galaxy.
