The galaxy appears to be a relatively smooth, elliptical type, exhibiting a centrally concentrated luminosity profile. There is a noticeable color gradient, transitioning from a yellowish-white core to a slightly redder outer halo. The overall shape is moderately elongated, but not highly cigar-shaped. There is no obvious evidence of strong spiral arm structure or active star formation regions within the galaxy, although the image resolution limits the ability to detect fine details. The galaxy appears relatively isolated with no signs of a major merger or strong tidal disturbances, although there are some minor asymmetries in the outer halo, perhaps suggesting a previous minor interaction or accretion event. These asymmetries could also be artifacts of image processing or noise. The smoothness and color suggest an older stellar population dominating the light output.
