The galaxy presents a generally smooth, elliptical morphology. It appears elongated, with a cigar-like shape, suggesting it may be an E4-E7 type elliptical. The central region exhibits a slightly brighter, concentrated luminosity. There is a color gradient noticeable, shifting from yellowish-white at the core to slightly reddish hues towards the outer edges. This might indicate an older stellar population dominating the outer regions. There does not seem to be any evidence of spiral arms or a prominent disk structure. No significant tidal disturbances or nearby companion galaxies are observed, implying a relatively isolated system that is undisturbed. There appears to be some red shift visible in the redder regions, which could indicate star forming regions.
