The galaxy presents a generally smooth, elliptical morphology, exhibiting a high degree of roundness. There is little evidence of strong spiral arm structure or other significant features. The galaxy's light profile indicates a relatively even distribution, with a central bulge that is moderately bright. The object shows a color gradient, appearing bluer in the central region, transitioning towards redder hues in the outer regions. This could potentially indicate ongoing star formation within the central part of the galaxy, with an older stellar population dominating the outskirts. No significant tidal disturbances or other signs of recent mergers are immediately apparent, although some minor distortions cannot be ruled out at this resolution. Based on the smooth appearance and color distribution, a classification of early-type galaxy appears appropriate. Further spectroscopic analysis is required to confirm star formation rates and stellar population characteristics.
