The galaxy exhibits a distinct elongated, cigar-like morphology, appearing as a prolate spheroid when viewed from our perspective. The central region is characterized by a bright, concentrated luminosity profile, suggesting a relatively high stellar density or active galactic nucleus. Proceeding outward from the core, the luminosity gradually diminishes, transitioning to a more diffuse halo. The overall color is a warm yellowish-orange hue, indicative of an older stellar population dominated by redder giants, though a slight gradient toward bluer colors on the galaxy's edges may indicate some ongoing, albeit subdued, star formation. There is no clear evidence of spiral arm structure or a prominent disk. The overall structure appears largely undisturbed, with only minimal suggestions of tidal features or recent merger activity. The galaxy presents a smooth texture.
