The galaxy presents as a relatively smooth, elliptical-like structure. Its core is distinctly brighter than the surrounding regions, suggesting a concentration of older stars and possibly a supermassive black hole at the galactic center. The overall color appears to be skewed towards the redder end of the spectrum, indicating an older stellar population with lower levels of on-going star formation. There is some evidence of a slightly extended halo, though the limited resolution makes it difficult to discern any detailed features within it. There does not appear to be any obvious spiral arm structure or significant dust lanes. The galaxy appears generally undisturbed, with no clear signs of ongoing or recent major merger events.
