The galaxy presents a smooth, elliptical morphology with a noticeable central bulge. The light distribution suggests a relatively homogenous stellar population, with the highest concentration of light emanating from the core, gradually fading outwards. There is little to no evidence of spiral arms, dust lanes, or active star formation regions. The galaxy appears somewhat elongated. The color profile indicates a mature stellar population, with a yellowish-red hue dominating the overall appearance. There are no signs of significant tidal disturbances or interactions with neighboring galaxies.
