The galaxy presents a generally smooth morphology, appearing largely featureless with a somewhat elliptical shape. The light distribution suggests it is not perfectly round, tending towards an 'in between' shape rather than a cigar shape. The central region exhibits a higher concentration of light, which fades gradually toward the outer edges. The color profile appears to shift from a slightly yellower hue in the core to bluer tones in the outer regions, possibly indicating a population of younger, bluer stars in the outskirts relative to a population of older, redder stars near the galaxy's center. There is no obvious evidence of major mergers or significant tidal disturbances in its immediate vicinity, which are features that would disrupt the smooth morphology of the object. Faint and extended outskirts give the appearance that this galaxy is larger than initially measured.
