The galaxy presents a slightly elongated morphology. It exhibits a central, concentrated region suggestive of a bulge, surrounded by a fainter, more diffuse disk. The disk appears somewhat disturbed, with subtle irregularities. The color profile suggests a mixture of stellar populations, with bluer tones prevalent in the disk, indicating recent or ongoing star formation, and a slightly redder central bulge. This object has a redshift of 0.043210, and is calculated to be approximately 3.7 kpc in radius. The estimated stellar mass is quite low, while its star formation rate indicates minimal ongoing activity, which is consistent with the observed morphology. There is a suggestion of minor gravitational interaction or recent merger activity within the disk.
