The observed galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing more rounded than elongated. There is a suggestion of a slight disturbance in its structure, possibly indicating a minor gravitational interaction, although no clear merger features are distinctly visible. The galaxy's color profile suggests the presence of an older stellar population, but also a non-negligible rate of star formation. The galaxy appears as an isolated object, residing in a relatively sparse region of space.
