This galaxy exhibits a smooth, elliptical morphology, with a relatively high degree of central concentration. It is elongated in shape, approaching a cigar-like appearance, suggesting a classification leaning towards an E4-E5 on the Hubble sequence. The light profile displays a gradual decline in intensity from the core outwards, lacking any prominent spiral arm structures or distinct features. The core appears to have a yellowish tint, while the outer regions display a subtly redder hue, hinting at an older stellar population dominating the outskirts. There appears to be a low probability of ongoing or recent major merger activity, as the galaxy does not show significant tidal tails, distorted isophotes, or multiple nuclei, although some minor disturbance may be present. The galaxy is unresolved, lacking the resolution to distinguish individual star-forming regions or dust lanes. Overall, the observed characteristics are consistent with a passively evolving elliptical galaxy at a moderate redshift.
