The galaxy presents a roughly elliptical morphology, with a noticeable elongation along one axis, giving it a somewhat cigar-like shape. Its color profile suggests the presence of a mixed stellar population, exhibiting a generally bluer hue in the central region, hinting at ongoing or recent star formation. Fainter, redder regions are visible at the periphery, suggesting the presence of older stellar populations. The light distribution appears generally smooth with little to no discernable spiral arm structure or obvious dust lanes. There is a hint of asymmetry or minor disturbances in the outer regions, which could potentially be indicative of minor tidal interactions or a recent merger event. Overall, the galaxy is of intermediate size, and demonstrates a moderate redshift, suggesting that we are observing it at a significant cosmological distance.
