This galaxy presents as a relatively smooth, centrally concentrated object. The morphology leans towards elliptical, although it is not perfectly spherical. It appears slightly elongated. There's little evidence of prominent spiral arms or significant substructure such as strong dust lanes. The galaxy exhibits a diffuse, extended halo surrounding a brighter central region, suggesting a substantial stellar population. The color profile indicates a relatively quiescent system, with light predominantly in the redder end of the spectrum, hinting at an older stellar population and a low rate of ongoing star formation. There may be minor disturbances from another object or even a past merger. Based on the overall characteristics, the galaxy appears to be an elliptical galaxy at a moderate distance.
