The object appears to be a galaxy exhibiting a predominantly smooth morphology. The light distribution suggests an elliptical shape with a high degree of roundness. There is no obvious spiral structure or prominent disk component discernible. The galaxy appears to be relatively isolated, without indications of major ongoing mergers or significant tidal disturbances, although a companion object is observed nearby. The dominant color is yellowish-orange, possibly indicative of an older stellar population with a low rate of star formation, although some level of star formation does seem to exist.
