The galaxy presents as a somewhat elongated, elliptical structure, characterized by a relatively smooth and diffuse light distribution. Its central region exhibits a notably bright and concentrated luminosity, appearing with a yellowish hue, indicative of an older stellar population. Moving outwards from the core, the light intensity gradually decreases, fading into the surrounding darkness. The galaxy's overall form suggests a flattened spheroid, leaning towards a more cigar-shaped appearance. There may be some minor signs of gravitational disturbance.
