The galaxy presents an elongated morphology, appearing somewhere between elliptical and lenticular. Its light profile suggests a relatively smooth, centrally concentrated bulge dominating the overall structure. The central region exhibits a bright, yellowish-white hue, indicating a population of older stars, possibly with ongoing or recently ceased star formation. Fainter and redder, extended emission is visible along the major axis, suggesting the presence of a disk component, though not prominently defined. There is no clear evidence of spiral arms or significant dust lanes. The object exhibits characteristics that could classify it as a galaxy with a substantial spheroidal component and a less defined disk. Some disturbance or interaction cannot be ruled out due to slight asymmetry.
