The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. A bright, concentrated central bulge is evident, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The galaxy appears relatively round with no obvious disc structure. Faint, diffuse extensions surround the central bulge, gradually fading into the background. There's a slight hint of bluer regions in the outer parts, potentially indicating some ongoing star formation, though at a relatively low rate. No significant signs of tidal disturbances or mergers are immediately apparent. The galaxy appears relatively isolated and undisturbed.
