The galaxy presents an elliptical morphology, appearing somewhat elongated and cigar-shaped. It exhibits a smooth, featureless structure with a concentration of luminosity toward the center, suggesting a prominent bulge. The color profile indicates a redder hue, which may indicate an older stellar population with ongoing star formation. There is some sign of minor tidal disturbances, possibly indicating a minor merger event in its past. It does not present any definitive spiral arm structure in this observation. Based on its estimated size of approximately 6.7 kpc, it is smaller than our Milky Way.
