The galaxy presents as an elongated, cigar-shaped structure with a notable central bulge. The core exhibits a high surface brightness, indicating a concentrated region of luminous matter. Progressing outward from the core, the luminosity gradually diminishes. The color profile appears to be relatively uniform, with a yellow-orange hue predominating. There is little evidence of distinct spiral arm structures or significant dust lanes. No clear indications of ongoing major merger activity are apparent, although subtle asymmetries or minor disturbances in the outer regions cannot be ruled out based solely on this image. The overall morphology suggests a system dominated by an older stellar population with a relatively low rate of current star formation.
