This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated, bright central bulge that transitions smoothly into a more diffuse outer region. The galaxy presents with a generally rounded morphology, displaying no prominent disk structures or spiral arms. There are no obvious signs of major mergers or significant tidal disturbances in its immediate vicinity; however, subtle asymmetries in the outer regions cannot be entirely ruled out. The color profile suggests a population of older stars dominating the light output, particularly in the central regions. The apparent redder hues towards the center may indicate a higher concentration of evolved, red giant stars. Fainter, bluer colors are observed in the outer regions, potentially indicating a younger stellar population or ongoing, but relatively low-level, star formation. The galaxy shows a degree of elongation, but overall maintains a round shape.
