The galaxy presents as a relatively smooth object with an elongated, cigar-like shape. Its central region displays a higher concentration of light, appearing brighter and more defined than the outer regions. The light distribution fades gradually from the center outward, suggesting a spheroidal or elliptical morphology. There are no obvious spiral arms or distinct dust lanes visible within the observed light. The galaxy's structure appears largely undisturbed, with no indication of major mergers or significant tidal interactions. Faint irregularities on the edges suggest potential minor disturbances or faint features within the galaxy's halo.
