The galaxy presents as a relatively smooth, centrally concentrated object with a predominantly elliptical morphology. A slight elongation is visible. There is a central, compact core displaying a bright bluish-white coloration, suggestive of a possible active galactic nucleus or a region of intense, obscured star formation. The surrounding region exhibits a reddish hue, indicating the presence of older stellar populations or dust obscuration. The overall structure does not show significant signs of major disturbances or tidal interactions, although some subtle irregularities in the outer isophotes cannot be entirely ruled out at this resolution. Based on the colors, the galaxy likely has a modest star formation rate and specific star formation rate. The galaxy appears to be of intermediate mass.
