The galaxy presents a generally smooth morphology, suggestive of an elliptical classification, though a subtle disk component cannot be entirely ruled out. Its shape appears to be moderately elongated, resembling a cigar shape. There is a concentration of light toward the center, potentially indicating an older stellar population. The overall color appears to be more muted than that of a spiral galaxy, suggesting less active star formation. No signs of major mergers or significant tidal disturbances are visible. There may be some minor disturbances. 
