The galaxy presents a largely smooth, elliptical morphology with a dominant central bulge. The light distribution is highly concentrated, exhibiting a gradual decline in intensity from the core outwards. No distinct spiral arm structures or prominent dust lanes are discernible. The overall color appears yellowish-orange, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no visible evidence of any major mergers or significant tidal disturbances. The galaxy appears nearly circular.
