The galaxy presents as a somewhat elliptical structure, with a major axis oriented roughly horizontally in the frame. The overall light distribution appears centrally concentrated, with a gradual decrease in surface brightness extending outwards. The color is generally homogenous, with a slightly yellow hue, indicating a relatively older stellar population compared to galaxies with strong blue color indicating active star formation. There are subtle irregularities in the light distribution, hinting at possible faint spiral arm segments or tidal features, although these are not sharply defined. There is no prominent central bulge. There may be some minor interaction with nearby objects, but this is not clearly indicated in the galaxy's morphology. Overall, the galaxy exhibits characteristics of a relatively quiescent system, possibly undergoing a slow rate of star formation. The apparent size of the galaxy suggests it is not a dwarf galaxy. Its redshift shows that it is relatively distant.
