The galaxy presents as a single, luminous, and relatively smooth object. Its morphology appears to be elliptical, with the overall shape exhibiting a slightly elongated, cigar-like form. The central region shows a high concentration of light, suggesting a dense nucleus. A smooth gradient in luminosity is observed from the core outwards, transitioning into a more diffuse halo. The color profile indicates a population of older stars, with a yellowish-red hue. There is no clear evidence of spiral arms or significant dust lanes within this galaxy, indicating a more quiescent state in terms of star formation. No signs of active galactic nuclei (AGN) activity are observed. There is a very slight possibility of a faint tidal feature, but no apparent signs of an ongoing or recent major merger event. Overall, this is a moderately massive galaxy displaying properties consistent with a relatively evolved system.
