The galaxy presents as a central bulge dominating its overall structure, with an elliptical appearance. Its shape is somewhere between round and elongated. The core exhibits a high surface brightness, indicating a dense concentration of stars. The bulge has a smooth appearance, showing some radial symmetry, suggesting a relatively relaxed distribution of stars. Hints of a faint disc surrounding the central bulge are noticeable. The spiral arms, if present, are not well defined in this image. The galaxy does not exhibit any major signs of strong tidal disturbance, or evidence of a recent merger. There is evidence of some star formation occurring within the galaxy. Overall, the galaxy shows characteristics of a moderately massive galaxy with intermediate star formation activity.
