The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color profile indicates an older stellar population, as evidenced by the yellowish-red hue dominant in the central regions. There's a slight flattening of the galaxy along its major axis, suggesting a possible, though subtle, disk component or the effects of rotation. No distinct spiral arms or dust lanes are visible. The overall appearance suggests a galaxy that is not actively forming stars at a high rate. There are some faint hints of bluer color surrounding the nucleus, suggesting that there may still be a small level of star formation present. The galaxy appears to be isolated with no obvious signs of ongoing merger activity or tidal interactions with other galaxies.
