The galaxy presents as an elongated, cigar-shaped form. Its central region appears relatively smooth, with a gradual fading towards the edges. The color profile suggests a population of older stars, exhibiting a reddish-yellow hue. There is no prominent evidence of ongoing star formation, as indicated by the absence of bright blue regions or HII regions. The galaxy's structure appears undisturbed, with no signs of tidal tails, mergers, or major distortions in its morphology. Based on its characteristics, it is likely an elliptical or lenticular galaxy viewed edge-on.
