The galaxy appears as a moderately sized, somewhat elongated structure. The central region exhibits a smooth, diffuse appearance, suggesting a relatively high degree of symmetry. The overall color profile indicates a population dominated by older stars, with a redder hue compared to younger, bluer star-forming regions. There is a hint of a disk like structure but it could be more that the galaxy has a cigar shape. Faint and seemingly undisturbed, it appears to be undergoing relatively low levels of star formation. The galaxy does not exhibit strong signs of recent or ongoing mergers or major tidal disturbances.
