The galaxy presents as a centrally concentrated object with a smooth morphology. There is a suggestion of a slight ellipticity, with the galaxy appearing somewhat elongated rather than perfectly spherical. The color profile indicates a dominant yellow-orange hue, potentially suggestive of an older stellar population. There is no apparent spiral structure or evidence of significant dust lanes visible. A slight bluer tint is perceptible on the very edge of the galaxy but not indicative of high star formation. The overall impression is that of a relatively quiescent galaxy.
