The galaxy appears to be an elliptical type, exhibiting a generally smooth, featureless morphology. The overall shape is elongated, with a cigar-like appearance. The galaxy presents a radial color gradient, transitioning from a bluer hue in the outer regions to a more pronounced reddish-orange core. This color shift suggests a stellar population gradient, where the outer regions may contain a higher proportion of younger, bluer stars, while the core is dominated by older, redder stars. There are subtle indications of possible minor disturbances or interactions, although the overall structure remains largely undisturbed. The galaxy appears relatively isolated, without any obvious signs of major ongoing merging activity.
