The galaxy presents as a moderately luminous object with an apparent smooth morphology. Its shape appears generally elliptical, with a slight deviation towards a cigar-like form. The color profile is dominated by redder hues, indicative of an older stellar population and reduced recent star formation activity. There is evidence of a possible minor disturbance in its structure, though the dominant impression is one of relative dynamical quiescence. The overall structure does not suggest a recent major merger, though minor tidal interactions cannot be ruled out. The galaxy exhibits a concentrated central bulge, which could indicate the presence of a supermassive black hole at its center.
