The galaxy presents a generally smooth and rounded morphology, with a dominant central bulge. There is little evidence of spiral arm structure or prominent features such as dust lanes. The light profile appears to be relatively uniform, suggesting a lack of ongoing major star formation. A slight elongation is discernible, but it deviates only subtly from a circular form. Overall, the galaxy appears consistent with an elliptical galaxy, although the possibility of a face-on spiral galaxy with a large bulge and minimal star formation cannot be definitively ruled out with this image alone. Further spectroscopic analysis is needed to determine the stellar population and confirm the galaxy's classification.
