The galaxy presents a predominantly smooth morphology, appearing largely elliptical in shape. There is a subtle elongation, suggesting a possible deviation from perfect sphericity towards a more cigar-like form. No distinct spiral arms or bar structures are discernible. There does not appear to be any major merging activity or substantial tidal disturbances in progress. The color profile indicates a relatively red hue, which may suggest an older stellar population and a lower rate of ongoing star formation. Its overall structure implies a relatively evolved system, consistent with a lenticular or elliptical classification.
