The galaxy presents a primarily smooth morphology, with a high degree of central concentration. The light profile suggests a fairly even distribution, lacking strong spiral arm features, but there is a slight asymmetry on its right side. The color distribution is relatively uniform throughout most of its structure, appearing with a yellowish hue. Based on this color, the galaxy is likely composed of an older stellar population. There is also some indication of ongoing interaction. A distinct extension is present to the lower right of the galaxy's core, perhaps indicating tidal disturbances caused by a minor merger.
