This galaxy appears to be a relatively smooth, elongated system. It is characterized by a centrally concentrated luminosity profile. The object exhibits a cigar-like shape, suggesting it is an edge-on disk galaxy or an elliptical galaxy with some degree of elongation. There is no evidence of strong spiral arm structure or prominent dust lanes visible in this image. There may be a faint disk component with an inclination near 90 degrees to our line of sight. There is no indication of a major ongoing merger or strong tidal disturbance, although the possibility of minor gravitational interactions or internal disturbances cannot be ruled out. Overall, the galaxy's morphology is consistent with a relatively quiescent system.
