The galaxy appears as a moderately bright, elliptical-like object with a smooth, diffuse morphology. The central region exhibits a concentrated luminosity profile, indicative of a bulge. There is a subtle color gradient, transitioning from a yellowish-white core to a slightly bluer hue towards the outer regions. The overall shape is somewhat elongated but generally lacks any distinct spiral arm features or irregular structures. The galaxy does not appear to be undergoing a major merger or exhibiting signs of significant tidal disturbances, although minor asymmetrical features may be present. Based on the color and morphology, the galaxy likely consists of an older stellar population with a relatively low current star formation rate.
