This galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a concentrated luminosity, appearing significantly brighter and displaying a yellowish-orange hue, potentially indicative of an older stellar population. The outer regions fade in intensity, showcasing a smoother texture. It appears to lack distinct spiral arms or prominent features. There are no visual signs of ongoing major merging events, though subtle disturbances cannot be ruled out. The overall morphology suggests a galaxy leaning towards an elliptical classification, although some disk-like properties are present. The estimated redshift indicates a considerable distance from our vantage point. Its color suggests that the galaxy may have a relatively low star formation rate.
