The galaxy appears as an elongated, smooth object with a concentrated central bulge. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. Fainter, bluer tinges surround the core, which may indicate pockets of more recent star formation, though these are not clearly resolved. The overall morphology is suggestive of an elliptical or lenticular galaxy, with a smooth light distribution. There is no apparent evidence of spiral arms or significant dust lanes. The galaxy shows a high degree of axial ratio, leaning towards an elliptical classification. There are no clear signs of any ongoing major merger activity or significant tidal disturbances based on the light distribution.
