The galaxy appears to be relatively compact, approximately 3 arcseconds in diameter. The overall morphology suggests a somewhat smooth structure, although there appears to be a slight asymmetry. There is a significant concentration of light in the central region, possibly indicating a galactic bulge or active galactic nucleus. The color profile reveals a bluer hue in the central region, suggesting the presence of younger, hotter stars or ongoing star formation. There is a fainter, reddish-orange extension to the right of the main body, potentially indicative of a tidal tail or a region of older stellar populations and dust. The apparent disturbances suggest a possible minor merger event in the galaxy's recent history. Overall, the galaxy exhibits properties of both elliptical and spiral galaxies, potentially representing an intermediate stage in galactic evolution or a disturbed system.
