The galaxy presents as a moderately luminous, elliptical-like structure. Its overall shape is somewhat elongated, exhibiting a cigar-like appearance. The central region displays a concentrated brightness, suggesting a prominent galactic nucleus. The color profile transitions from a yellowish hue in the core to a reddish-orange periphery, possibly indicating an aging stellar population throughout. There is a faint hint of blue-green tint on one side of the galaxy which suggests there is a small amount of recent star formation occurring within it. There is no clear evidence of spiral arms or a well-defined disk. The galaxy appears relatively undisturbed, lacking any major signs of ongoing mergers or tidal interactions, although there is a very slight asymmetry on one side, which indicates it may have merged with a much smaller galaxy in the past.
