The galaxy presents as a largely featureless, elliptical or lenticular structure. The core region is distinctly brighter, exhibiting a concentrated luminosity. The overall color profile indicates a bias towards redder wavelengths, possibly indicative of an older stellar population with limited ongoing star formation. The galaxy's shape is somewhat elongated. There is no apparent evidence of spiral arms or a prominent disk structure. There's no obvious signs of interaction or ongoing merger activity with other galaxies. There is some minor disturbances in the image, which suggests that there is possibly a merging event happening. The galaxy's smooth morphology suggests a dynamically relaxed system.
