The galaxy presents as a cigar-shaped, elongated structure, suggesting it is likely an elliptical galaxy viewed at an angle. Its core exhibits a bright, yellowish-white hue, potentially indicating an older stellar population concentrated toward the center. Fainter, diffuse bluish regions extend outward from the central bulge, hinting at the presence of some younger, bluer stars and possibly ongoing, albeit low-level, star formation within the galaxy's outskirts. There is no evident spiral arm structure. There are no signs of a significant merger or tidal disruption in the immediate vicinity.
