This galaxy presents as a relatively small, elongated system. Its central region exhibits a brighter, somewhat diffuse glow, suggesting a concentration of stars or active galactic nucleus activity, though this requires spectroscopic confirmation. Moving outwards from the center, the light fades gradually, showing a hint of a disk-like structure, but without clearly defined spiral arms. The overall color is a mix of blue and red, indicating a mix of stellar populations and potentially ongoing star formation. The galaxy’s shape is significantly elongated, appearing cigar-shaped, lacking a strong bulge component. There is a minor irregularity in its structure which may be from a minor disturbance, but no clear signs of a major merger are visible. It appears to be a relatively isolated galaxy within its immediate vicinity.
