The galaxy presents as a moderately luminous object with a distinct elliptical morphology. Its core exhibits a concentrated, smooth distribution of light, characterized by a yellowish-orange hue, suggesting an older stellar population. There is a subtle gradient towards bluer colors on the outer edges of the galaxy which may be a result of younger stars or less dust absorption on the edges of the galaxy.

Two prominent features are near the main galaxy. The object above the galaxy is much smaller and bluer, and the object below the galaxy is also smaller but more orange in color. These may be the results of tidal disturbances or galaxies in the same galaxy group. There are no clear signs of a spiral arm structure, and dust lanes or other significant morphological features are not apparent. The overall smooth appearance and color profile indicate a galaxy undergoing a relatively quiescent phase of stellar evolution. Further spectroscopic analysis would be beneficial to confirm the stellar population and star formation history.
