This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light distribution. Its shape is elongated, with the major axis significantly longer than the minor axis. There is a bright central bulge that is highly luminous. The galaxy has a redder overall color, suggesting an older stellar population with limited ongoing star formation. Faint extensions of light are visible at the edges of the galaxy, giving it a diffuse appearance and gradual falloff in brightness. No distinct spiral arms or prominent dust lanes are discernible. There is no strong evidence of any major ongoing merging activity. Any minor disturbances are difficult to observe at this resolution.
