The galaxy presents a generally smooth, elliptical morphology. Its light profile appears relatively uniform, with a gradual decrease in intensity from the center outwards. The shape can be described as tending towards "cigar-shaped". There are no apparent spiral arms or prominent dust lanes visible. The color is fairly homogenous across the galaxy, with a slight tendency towards redder hues. There are no obvious signs of active galactic nuclei activity or strong star-forming regions, which supports the lack of significant blue color. Overall, the galaxy gives the impression of being a relatively quiescent system, with a light signature consistent with an older stellar population. There is also no evidence of a major merger event in its recent past, though there seems to be some minor distortion in its shape. 
