The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, exhibiting a somewhat elongated, cigar-like morphology. There is a slight indication of a disk. The color profile indicates a predominantly older stellar population, shown by the yellow-orange hue, and the overall luminosity suggests that the rate of star formation is relatively low. There are no obvious signs of recent mergers or major disturbances, though a minor tidal interaction cannot be ruled out. The galaxy’s estimated size seems to be moderately compact, spanning approximately 3.5 kpc. Overall, the galaxy presents as an evolved, relatively quiescent system.
