The galaxy presents a generally smooth, elliptical morphology. There is a slight elongation, more consistent with an in-between roundedness, rather than a perfectly circular or cigar shape. The central region exhibits a concentrated luminosity profile, displaying a yellow-ish color, which suggests a population of older stars. Progressing outwards from the central region, the luminosity gradually decreases, showing a faint halo or envelope. There is no clear presence of defined spiral arms or significant dust lanes; the structure appears largely featureless and smooth. No distinct signs of active galactic nuclei or significant ongoing star formation activity are immediately obvious from the broadband image. Furthermore, it does not exhibit any signs of major mergers or tidal disturbances. There is only minimal structure or complex features detected.
