The galaxy appears as a moderately bright, elliptical or lenticular system. Its morphology suggests it is primarily composed of an older stellar population with little to no discernible spiral arm structure. The color is generally redder in appearance, consistent with a population of older, cooler stars. The galaxy's light is fairly smooth and centrally concentrated, suggesting a significant bulge component. There's little evidence of ongoing star formation activity, and the overall shape is more elongated than circular, but not cigar shaped. There is no obvious sign of a recent major merger or tidal disturbance. The galaxy appears relatively isolated, with no other major galaxies in close proximity exhibiting strong gravitational interaction.
