The galaxy presents an overall elongated, cigar-like morphology. It exhibits a central, luminous region suggesting a dense galactic nucleus. Proceeding outwards from the nucleus, a smooth gradient in luminosity is observed, characteristic of a relatively undisturbed system.

The galaxy's color profile indicates a bluer hue in the outer regions, suggesting ongoing or recent star formation activity, especially at one end. The core, while still generally bluish, appears slightly less intense than the lower regions. This could be caused by older stellar populations and/or dust obscuration, but it is difficult to tell without more data. The structure appears to be a disk galaxy, viewed at an angle. There is no evidence of strong tidal distortions or a major merger. There is an area on the lower side that is brighter and may indicate a merging dwarf galaxy, but the area could also just be an area of higher star formation.
