The galaxy appears as a compact, elliptical-like object. It has a smooth overall structure, with a near-spherical shape. The color distribution is predominantly bluish, indicating the presence of relatively young stars. There is no apparent spiral arm structure or a distinct galactic bulge. A slight asymmetry in the color distribution and a small area of higher concentration on one edge may indicate a possible minor disturbance, perhaps due to a small galactic interaction or tidal stripping. However, the galaxy does not appear to be a strong merger. Based on the estimated distance and observed brightness, this galaxy would be considered a luminous object with significant mass. There appears to be ongoing but relatively low levels of star formation.
