The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. The color profile suggests a generally older stellar population, characterized by a yellowish-red hue, indicative of evolved stars and a relatively low rate of ongoing star formation. There's a slight elongation to the galaxy's shape, suggesting it is not perfectly spherical. No distinct spiral arms or prominent dust lanes are discernible within the resolution of the image. There's a very slight asymmetry observable, which may be indicative of a minor tidal interaction or past merger event.