The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. The light profile suggests a spheroid-dominated system, with a notable lack of distinct spiral arm structures or prominent dust lanes. The galaxy appears somewhat elongated, deviating slightly from a perfectly circular form. There is a hint of a possible minor disturbance or interaction based on a slight asymmetry in the outer regions. Its color index indicates that the galaxy's stellar population might be comprised of older stars, although bluer light is visible near the center. Based on the data, there is very little in the way of current star formation taking place in this galaxy. There is no visible evidence of a major merger event, however, the galaxy has a slight asymmetry which could be the result of a prior minor disturbance or interaction.
