This galaxy appears to be a relatively small, elliptical galaxy. It has a smooth, diffuse light distribution, with no prominent spiral arms or dust lanes visible. The galaxy's shape is somewhat elongated, tending towards a cigar-like morphology. The core of the galaxy exhibits a slightly brighter and more concentrated region. The overall color of the galaxy is on the bluer side, suggesting a young stellar population. There is no definitive evidence of a major ongoing merger, though there might be a slight disturbance in the galaxy's morphology, potentially due to a minor interaction or recent accretion event. The rate of star formation is low, and the stellar population is dominated by older stars. The galaxy exhibits a noticeable halo extending beyond the main body.
