The galaxy presents a primarily smooth appearance, indicating a possible elliptical or lenticular morphology. There is evidence of a merging event or significant gravitational interaction, potentially with another galactic structure not fully resolved in this image. The galaxy exhibits a moderate degree of roundness, deviating slightly from a perfect sphere. The light distribution suggests an older stellar population with a redder hue, although some bluer regions are also visible. This potentially indicates regions of recent or ongoing star formation. There appears to be some internal structure and slight asymmetry in the galaxy's shape, likely due to the aforementioned gravitational interaction. This galaxy has an apparent size that places it at a moderate distance. The overall color and morphology suggest a relatively high mass object with a moderate rate of star formation.
