The galaxy presents as an elliptical morphology, exhibiting a generally smooth texture without prominent spiral arm structures. The core is bright, indicating a high concentration of stars. The galaxy displays a slight elongation, deviating from a perfectly circular form. The color profile suggests a stellar population that is relatively old, with a redder hue. There appears to be no current or recent major merger activity, but possibly there is a minor interaction with a neighbor. There is a distinct lack of dust lanes or other obscuring features within the galactic disk, supporting the assessment of an older stellar population and relatively low levels of active star formation.