The galaxy presents as a somewhat elongated, cigar-shaped structure. The central region exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluish extensions emanate from the core along the major axis, indicating regions of more recent star formation. There appears to be a slight asymmetry in the distribution of the bluer light, possibly indicating a tidal interaction or recent merger event. The galaxy overall has a relatively smooth appearance, but there are minor disturbances that could possibly be merging.
