The galaxy presents as a slightly elongated, lenticular structure. It appears relatively smooth in texture, with a concentrated central bulge that graduates outward into a less defined disk. There is a noticeable color gradient, transitioning from a yellowish hue in the core to a slightly bluer tint in the outer regions of the disk. The axial ratio suggests a moderate inclination relative to our line of sight. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of recent major merger events, although there may be evidence of minor tidal interactions. The color profile suggests a population dominated by older stars, with a potentially small component of more recent star formation occurring within the disk. The galaxy is relatively compact in size.
