The galaxy presents as a moderately luminous object with a notable degree of central concentration. Its morphology is suggestive of an early-type galaxy, possibly an elliptical or lenticular, exhibiting a relatively smooth, spheroidal profile. There is a subtle hint of a disk-like structure, or perhaps a ring, surrounding the core, but it is not clearly defined. The galaxy does not show prominent spiral arms or strong features typically associated with actively star-forming regions. The color profile indicates a redder overall hue, consistent with an older stellar population and reduced ongoing star formation. There is no clear evidence of a major merger event, though some minor distortions or tidal features cannot be ruled out with this image resolution.
