The galaxy presents as a relatively compact, elliptical or lenticular system. Its morphology appears largely smooth, with a high degree of central concentration of light. A discernable bulge is evident, though no prominent spiral arm structures are visible. The galaxy exhibits an overall redder color, indicative of an older stellar population and potentially lower levels of ongoing star formation. The galaxy displays a somewhat elongated shape, resembling an cigar shape. There is no indication of major mergers or significant tidal disturbances in the image. The galaxy appears relatively isolated, without close companion galaxies that would suggest recent interactions or merging events.
