The galaxy appears to be a relatively smooth, elliptical galaxy, potentially of moderate mass. It exhibits a bright, concentrated central bulge that fades gradually into an extended halo. The galaxy's overall shape is more 'in-between' than distinctly round or cigar-shaped. The color profile suggests an older stellar population, with a yellow-red hue dominant throughout the galaxy. There is no clear evidence of distinct spiral arms or significant dust lanes. No major or minor mergers are obvious, but a very slight asymmetry is visible. Although it appears largely undisturbed morphologically, deeper analyses may reveal faint tidal features. The galaxy is actively forming stars, at a relatively low rate.
