The galaxy presents an elongated, cigar-shaped morphology. Its core exhibits a bright, concentrated luminosity, suggesting a relatively high stellar density in the central region. The overall color profile indicates a population dominated by older stars, with a notable lack of prominent blue regions typically associated with active star formation. Faint indications of spiral arm structure are potentially present, but largely obscured by the image resolution and viewing angle. There is no evidence of any significant ongoing merging activity or major disturbances in the galactic structure, though the possibility of a minor interaction cannot be ruled out. A smooth, featureless texture characterizes most of its visible components.
