The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that fades gradually into the outer regions. The color profile suggests an older stellar population, with a yellowish hue dominant in the core, indicating a lack of significant ongoing star formation. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy is largely undisturbed, showing no major signs of tidal interactions or recent merger activity. A very faint hint of bluer color might be present in the outer regions, suggesting a small amount of younger stars there, but it may also be image noise. Overall, the system presents as a well-evolved, early-type galaxy.
