The galaxy appears as a centrally concentrated elliptical, exhibiting a smooth and largely featureless morphology. The light is most intense in the core, fading gradually outward. The galaxy's shape appears to be slightly elongated, with an aspect ratio suggesting it is neither perfectly spherical nor highly flattened. There is no clear evidence of spiral arms, prominent dust lanes, or significant tidal features. The galaxy has an apparent angular size of 1.45 arcseconds, corresponding to a physical size of around 4.5 kpc. The color profile indicates a redder hue at the center, shifting towards a bluer hue in the outer regions, likely caused by ongoing star formation. This is also supported by estimates of log(SFR) of about 2.13 solar masses per year. There seems to be no major disturbances or ongoing mergers visible in the image.
