The galaxy appears to be an elongated, cigar-shaped system, viewed nearly edge-on. It exhibits a smooth, diffuse light distribution, lacking any distinct spiral arm structures or prominent dust lanes. The central region appears somewhat brighter and more concentrated than the outer regions. There is a slight hint of blueish hue, indicating the presence of some ongoing, albeit likely low-level, star formation activity. The overall morphology suggests a galaxy with a considerable amount of its star formation completed. There is no evidence of any significant merging activity or tidal disturbances. The observed structure implies a relatively evolved galaxy, potentially of early-type morphology.
