The galaxy presents a largely smooth morphology, with a high probability that it is smooth. Its shape appears more in-between than distinctly round or cigar-shaped, indicating a moderate ellipticity. There are no clear signs of major mergers or significant tidal disturbances affecting its overall structure.

The galaxy exhibits a relatively faint apparent magnitude, but when corrected for redshift, its absolute magnitude suggests a moderate luminosity. The estimated mass of the galaxy is significant, placing it within the range of a typical galaxy.

Based on its color indices, the galaxy's stellar population is likely dominated by older, redder stars, suggesting a relatively low star formation rate. The specific star formation rate, which normalizes star formation by stellar mass, further reinforces this impression of a quiescent galaxy, possibly with star formation largely shut down.
