The galaxy presents a predominantly smooth, elliptical morphology with a high degree of central concentration. Its color profile is consistent with an older stellar population, exhibiting a yellowish-orange hue indicative of a relatively passive galaxy with minimal ongoing star formation. The overall round appearance suggests a classification tending towards E0-E3 on the Hubble sequence. There is no apparent evidence of spiral arm structures, dust lanes, or tidal features, consistent with a lack of recent major mergers. The galaxy appears well-defined with a gradual decrease in luminosity moving outward from the center. Minor disturbances may be present, but are not pronounced in this image. The galaxy displays minimal features in the outer regions.
