The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape, although it does not look perfectly rounded. Its central bulge is prominent and exhibits a concentrated luminosity gradient, indicating a high stellar density within. There may be a faint disk component. The color profile is slightly redder than the galactic average, with minimal evidence of blue star formation regions. The galaxy does not show any clear signs of significant tidal disturbances or ongoing major mergers with other galaxies. The galaxy's overall structure suggests a relatively evolved stellar population and a lack of current high star formation activity. Some minor disturbances may be ongoing.
