This galaxy appears to be a luminous, compact object with a generally smooth morphology. Its color profile leans toward the redder end of the spectrum, implying a relatively older stellar population with reduced ongoing star formation. The galaxy exhibits an elliptical shape with a mostly even distribution of light across its surface. There is no significant evidence of spiral arms or a prominent disk structure. Instead, the light is concentrated towards the galaxy's center, creating a bright core. While the galaxy appears mostly undisturbed, subtle irregularities are visible, hinting at possible interactions or minor disturbances. Overall, the galaxy is a high mass elliptical galaxy with little current star formation. The morphology is that of a generally round object, possibly in the process of a merger.
