The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish hue, potentially indicating an older stellar population. The galaxy appears moderately elongated, with a slight departure from a perfectly circular shape. A faint, diffuse halo surrounds the central region, gradually fading into the background sky. There is little evidence of significant spiral arm structure or active star formation regions. The overall color profile suggests a galaxy with a relatively low ongoing star formation rate, possibly nearing a state of quiescence. No major tidal disturbances or merger events are apparent from the image.
